Refimprove date September 2009 Be X ray binaries BeXRB s are a class of high mass X ray binaries that consist of a Be star and a neutron star . The neutron star is usually in a wide highly elliptical orbit around the Be star. The Be stellar wind forms a disk confined to a plane often different from the orbital plane of the neutron star. When the neutron star passes through the Be disk, it accretes plenty of gas in a short time. As the gas falls onto the neutron star, a bright flare in hard X ray s is seen. LSI 61 303 LS I 61 303 LSI 61 303 is a periodic, radio emitting binary system that is also the gamma ray source, CG135 01. ref name Taylor cite journal author Taylor AR, Young G, Peracaula M, Kenny HT, Gregory PC title An X ray outburst from the radio emitting X ray binary LSI 61 303 journal Astron Astrophys. year 1996 volume 305 pages 817 24 bibcode 1996A&A...305..817T ref Using the ROSAT and VLA observatories, an X ray outburst with an 10 d duration was detected. ref name Taylor LSI 61 303 is a variable radio source characterized by periodic, non thermal radio outbursts with a period of 26.496 d. ref name Taylor The 26.5 d period has been attributed to the eccentric orbital motion of a compact object, probably a neutron star, around a rapidly rotating B0 Ve star, with a T sub eff sub 26,000 K and luminosity of 10 sup 31 sup watt s 10 sup 38 sup erg s sup 1 sup . ref name Taylor Photometric observations at optical and infrared wavelengths also show a 26.5 d modulation. ref name Taylor Of the 20 or so members of the Be X ray binary systems, as of 1996, only X Per and LSI 61 303 have X ray outbursts of much higher luminosity and harder spectrum kT energy kT 10 20 keV ... high mass X ray binaries such as SS 433 , Cygnus X 3 Cyg X 3 and Circinus X 1 Cir X 1 . ref name Taylor References reflist 2 DEFAULTSORT Be X Ray Binaries Category Binary stars Category X ray binaries Be X ray binaries Category Be stars Be X ray binaries star system stub pt Bin rio emissor de raio ... more details
Sygnus X can refer to Cygnus X star complex , a giant star formation region in the Milky Way galaxy Cygnus X music group , a trance music project by Matthias Hoffmann Cygnus X 1 disambiguation Cygnus X 2 Cygnus X 3 , one of the brightest X ray binaries dab ... more details
notability Products date December 2011 Binary recompiler is a software that takes executable Binary file binaries as input, analyzes the structure, applies transformations and optimizations, and outputs new optimized executable binaries. ref http www.eecs.umich.edu jringenb binary recomp.html umich.edu Binary Recompilation and Combined Compiler Architecture Enhancements Studies ref First introduced by Gary Kildall in the 1980s. citation needed date March 2012 See also Compiler Transcompiler Dynamic recompilation Binary translation References references Category Compilers Category Compiler construction Category Computer libraries ... more details
Apple s trademarks related to Universal binaries. ref http developer.apple.com softwarelicensing agreements ... based on Intel processors, which began shipping in 2006. Universal binaries typically include ... upon capabilities present only in OS X 10.6 or newer no longer require Intel PPC fat binaries. Additionally ... binaries. Presently, fat binaries would only be necessary for software that is designed to have backward ... general alternative solutions. The first is to simply provide two separate binaries, one compiled ... binaries or specifically compiled binaries are available see Rosetta software Rosetta . Universal binaries are larger than single platform binaries, because multiple copies of the compiled code must be stored ... of the resulting universal binary can be, and usually is, smaller than both binaries combined. They also ... to PowerPC in the mid 1990s. These dual platform executables were called fat binary fat binaries ... binaries even further, by allowing four architecture binaries to be created 32 and 64 bit for both ... part of the OS. Identifying universal binaries The Unix tt file command file tt command on OS X and several other Unix like systems can identify Mach O universal binaries and report which architecture ... OS X application that allows the user to slim down the fat universal binaries by removing the code ... Mac OS X Category Executable file formats Category Mac OS X ca Binari universal de Universal Binaries es Binario universal fr Universal binaries ko it Universal binary mr ... more details
Image Accretion disk.jpg 300px thumb Artist s impression of an X ray Binary X ray binaries are a class of binary star s that are luminous in X ray s. The X rays are produced by matter falling from one component, called the donor usually a relatively normal star to the other component, called the accretor , which is compact a white dwarf , neutron star , or black hole . The infalling matter releases gravitation al potential energy , up to several tenths of its rest mass, as X rays. Hydrogen nuclear fusion fusion releases only about 0.7 percent of rest mass. An estimated 10 sup 41 sup positron s escape ... Source Solved Maybe by John Borland 2008 ref Classification X ray binaries are further subdivided ... donor, not to the compact X ray emitting accretor. Low mass X ray binary Low mass X ray binaries LMXBs Soft X ray transient s SXTs Symbiotic variable star Symbiotic X ray binaries Super soft X ray source ... to Cataclysmic Variables CVs , NASA, 2006. ref SSSs , SSXB Intermediate mass X ray binaries Intermediate mass X ray binaries IMXBs High mass X ray binary High mass X ray binaries HMXBs Be X ray binaries Be X ray binaries BeXRBs X ray astronomy Analytical X ray astronomy Supergiant X ray binaries SGXBs ... X ray binaries unveiled by INTEGRAL ref ref http arxiv.org pdf 0809.3157 L. Sidoli, 2008 Transient ... X ray binaries that can house either a neutron star or a black hole Low mass X ray binary A low mass ... Evolutionary Binary Sequences for Low and Intermediate Mass X ray Binaries , Philipp Podsiadlowski ... and therefore easily detected. One of the most famous high mass X ray binaries is Cygnus X 1 ... luminous in the optical and X ray regions. Microquasars are sometimes called radio jet X ray binaries to distinguish them from other X ray binaries. A part of the radio emission comes from relativistic ... astronomy ep 135 x ray astronomy Astronomy Cast X ray Astronomy Category X ray binaries Category Binary stars Category Semidetached binaries Category Microquasars Category Astronomical X ray ... more details
copy to Wikibooks Cookbook South Side Cocktail is an alcoholic beverage that is commonly consumed during the summer months because it is refreshing and its deliciousness often goes undisputed. It is named after the South Side, Chicago South Side district of the city of Chicago, Illinois. The following recipe is for one cocktail and is used by the famed 21 Club in New York City. Ingredients 2 oz. vodka , gin , or rum white rum The juice of one lemon 2 tsp. of granulated sugar 1 tbsp of Fresh mint leaves Method Place ingredients in a cocktail shaker and shake vigorously to bruise the mint leaves Strain into a chilled collins glass filled with ice Enjoy and repeat References See Wikipedia Footnotes on how to create references using ref ref tags which will then appear here automatically http www.orient express.com binaries South 20Side tcm4 116330.pdf 21 Club Recipe Reflist External links http www.orient express.com binaries South 20Side tcm4 116330.pdf Categories Category Cocktails with vodka Category Cocktails with rum Category Cocktails with gin ... more details
A W Ursae Majoris variable is a type of eclipsing binary variable star . These stars are close binaries of spectral types F, G, or K that share a common envelope of material and are thus in contact with one another. They are termed contact binary contact binaries because the two stars touch and transfer mass and energy through the connecting neck, although astronomer R.E. Wilson argues that the term overcontact is more appropriate. ref name wilson2001 cite journal last1 Wilson first1 R. E. year 2001 title Binary Star Morphology and the Name Overcontact journal Information Bulletin on Variable Stars volume 5076 pages 1 bibcode 2001IBVS.5076....1W ref W Ursae Majoris variables are the most common variable stars in the present day Universe. About 1 percent of all stars belong to this group. The class is divided into two subclasses A type and W type L. Binnendijk, Veroeffentlichungen der Remeis Sternwarte zu Bamberg, Nr. 40., p. 36, 1965 A type W UMa binaries are composed of two stars both hotter than the Sun, having stellar classification spectral types A or F, and orbital period periods of 0.4 to 0.8 day. The W types have cooler spectral types of G or K and shorter periods of 0.22 to 0.4 day. The difference between the surface temperatures of the components is less than several hundred kelvin s. A new subclass was introduced in 1978 B type. The B types have larger surface temperature difference. In 2004 the H high mass ratio systems were discovered by Sz. Csizmadia and P. Klagyivik Astronomy and Astrophysics , Vol. 426, pp. 1001 1005 2004 . The H types have a higher mass ratio than math q 0.72 math math q math secondary s mass primary s mass and they have extra angular momentum . Their light curves differ from those of classical eclipsing binary eclipsing binaries , undergoing a constant ellipsoidal variation rather than discrete eclipse s. This is because the stars ... W Ursae Majoris variables Category Common envelope binary stars Category Eclipsing binaries Category ... more details
Orphan date April 2012 2MASS J21392676 0220226 is a brown dwarf 47 light years from earth. ref Andrew Fazekas. http news.nationalgeographic.com news 2011 09 110913 extreme storm brown dwarf star jupiter spot space science Colossal Storm May Rage on Jupiter like Failed Star . ref Its surface is thought to be host to a massive storm. ref Dean Praetorius. http www.huffingtonpost.com 2011 09 13 storm on a star brown dwarf n 960470.html Brown Dwarf May Be Host To Massive, Violent Mega Storm . The Huffington Post , 9 13 2011. ref It was discovered in the Two Micron All Sky Survey 2MASS . External links cite journal last1 Burgasser first1 Adam J. last2 Cruz first2 Kelle L. last3 Cushing first3 Michael last4 Gelino first4 Christopher R. last5 Looper first5 Dagny L. last6 Faherty first6 Jacqueline K. last7 Kirkpatrick first7 J. Davy last8 Reid first8 I. Neill last9 first9 year 2009 title SpeX Spectroscopy of Unresolved Very Low Mass Binaries. I. Identification of Seventeen Candidate Binaries Straddling the L Dwarf T Dwarf Transition journal The Astrophysical Journal volume 710 issue 2 pages 1142 arxiv 0912.3808 bibcode 2010ApJ...710.1142B doi 10.1088 0004 637X 710 2 1142 References references Category Brown dwarfs Category 2MASS objects pl 2MASS J21392676 0220226 ... more details
optically, in which case they are called visual binaries . Many visual binaries have long orbital periods .... They may also be detected by indirect techniques, such as spectroscopy spectroscopic binaries or astrometry astrometric binaries . If a binary star happens to orbit in a plane along our line of sight ... binaries , or, as they are detected by their changes in brightness during eclipses and transits, photometric binaries . If components in binary star systems are close enough they can gravitationally ... attain. Examples of binaries are Sirius and Cygnus X 1 of which one member is probably a black hole ... or interferometry interferometric methods are known as visual binaries . ref name Heintz12 ... astr162 lect binaries visual.html title Visual Binaries publisher University of Tennessee ... have not been ascertained to be either true binaries or optical double stars. ref http ad.usno.navy.mil ... for example, several spectroscopic binaries are also eclipsing binaries. Visual binaries A visual ... . The angular resolution of the telescope is an important factor in the detection of visual binaries ... binaries will be detected. The brightness of the two stars is also an important factor, as brighter ... name csep10 Spectroscopic binaries This section is linked from Redshift Sometimes, the only evidence ... effect Doppler shift of the stars spectral line s, the binaries detected in this manner are known as spectroscopic binaries . Most of these cannot be resolved as a visual binary, even with telescope s of the highest existing Angular resolution resolving power . In some spectroscopic binaries, spectral ... red and back again. Such stars are known as single lined spectroscopic binaries SB1 . The orbit ... a or i can be determined by other means, as in the case of eclipsing binaries, a complete solution ... Binary stars that are both visual and spectroscopic binaries are rare, and are a precious source of valuable ... together, usually too close to be detected as visual binaries. Binaries that are both visual ... more details
binaries is not common in operating system software there are several alternatives to solve the same ... code generally runs slower than native code. Applications released as fat binaries took up more ... mac runtimehtml RTArch 87.html archivedate March 7, 2004 ref Fat binaries were larger than programs ... drive usage. NeXT s Apple s Multi Architecture Binaries NeXTSTEP Multi Architecture Binaries Fat binaries were a feature of NeXT s NeXTSTEP OPENSTEP operating system, starting with NeXTSTEP 3.1 in NeXTSTEP, they were called Multi Architecture Binaries . Multi Architecture Binaries were originally ... s Mac OS X 2001 , and NeXT s Multi Architecture Binaries continued to be supported by the operating system. Under Mac OS X, Multi Architecture Binaries can be used to support multiple variants of an architecture ... web author Apple Computer title Universal Binaries and 32 bit 64 bit PowerPC Binaries in the Mac OS ... to offer both PPC and Intel binaries, using Universal binaries. The obvious cost of Universal ... for the Intel and or PowerPC architecture. Universal binaries created with this in mind can contain ... 64 64 bit x86 . Linux FatELF Universal Binaries for Linux http icculus.org fatelf FatELF is a Fat ... of binaries with support for multiple kernel Application binary interface ABIs and versions. FatELF ... FatELF Universal Binaries for Linux. url http icculus.org fatelf benefits date accessdate 2010 07 ... first Thom ref DOS Combined COM style binaries for CP M 80 and DOS CP M 80 executables for the Intel ... 8086 binaries. In both cases programs are loaded at offset 100h and executed by jumping to the first ... to avoid this methods have been devised to build fat binaries which contain both a CP M 80 and a DOS ... fatelf FatELF Universal Binaries for Linux DEFAULTSORT Fat Binary Category Executable file formats ... more details
About contact binary stars asteroids Contact binary asteroid In astronomy , a contact binary is a binary star system whose component stars are so close that they touch each other or have merged to share their gaseous envelopes. A binary system whose stars share an envelope may also be called an overcontact binary. ref http www.daviddarling.info encyclopedia C contact binary.html contact binary , David Darling, The Internet Encyclopedia of Science . Accessed on line November 4, 2007. ref ref http www.daviddarling.info encyclopedia O overcontact binary.html overcontact binary , David Darling, The Internet Encyclopedia of Science . Accessed on line November 4, 2007. ref ref pp. 51&ndash 53, An Introduction to Astrophysical Fluid Dynamics , Michael J. Thompson, London Imperial College Press, 2006. ISBN 1 86094 615 1. ref Almost all known contact binary systems are Binary star Eclipsing binaries eclipsing binaries ref p. 231, Stellar Rotation , Jean Louis Tassoul, Andrew King, Douglas Lin, Stephen P. Maran, Jim Pringle, and Martin Ward, Cambridge, UK, New York Cambridge University Press, 2000. ISBN 0 521 77218 4. ref eclipsing contact binaries are known as W Ursae Majoris variables , after their type star, W Ursae Majoris . ref p. 19, Double and Multiple Stars and how to Observe Them , James Mullaney, New York, London Springer, 2005. ISBN 1 85233 751 6. ref Contact binaries are sometimes confused with common envelope s. However, whereas the first refers to a stable configuration of two touching stars in a binary with a typical lifetime of millions to billions of years, the latter describes a dynamically unstable phase in binary evolution which either expels the stellar envelope or merges the binary in a timescale of months to years. See also Binary star Binary system astronomy Common envelope Contact binary asteroid References Reflist Astronomy stub Category Binary stars Category Common envelope binary stars es Estrella binaria de contacto fr Binaire contact ja pl ... more details
starbox short constell Andromeda constellation Andromeda name 47 Andromedae type A1m ref name SIMBAD SIMBAD, http simbak.cfa.harvard.edu simbad sim basic?Ident 47 Andromedae&submit SIMBAD search 47 Andromedae accessed 4 4 2012 ref ra RA 01 23 40.61627 ref name SIMBAD dec DEC 37 42 53.7861 ref name SIMBAD 47 Andromedae 47 And is a spectroscopic binary spectroscopic binary star binary star in the constellation Andromeda constellation Andromeda . Its apparent magnitude is 5.60. References reflist Stars of Andromeda Category Andromeda constellation Category Spectroscopic binaries Category A type stars Category Flamsteed objects Andromedae, 47 binary star stub ca 47 Andromedae uk 47 ... more details
starbox short constell Aquarius constellation Aquarius name 32 Aquarii type A3m ref name SIMBAD SIMBAD, http simbak.cfa.harvard.edu simbad sim basic?Ident 32 Aquarii&submit SIMBAD search 32 Aquarii accessed 25 March 2012 ref ra RA 22 04 47.42234 ref name SIMBAD dec DEC 00 54 22.8311 ref name SIMBAD 32 Aquarii 32 Aqr is a spectroscopic binary spectroscopic binary star binary star in the constellation Aquarius constellation Aquarius . Its apparent magnitude is 5.29. References reflist Stars of Aquarius Category Aquarius constellation category Spectroscopic binaries Category A type stars Category Flamsteed objects Aquarii, 32 binary star stub ca 32 Aquarii id 32 Aquarii ... more details
starbox short constell Aquarius constellation Aquarius name 17 Aquarii class M0III ref name SIMBAD SIMBAD, http simbak.cfa.harvard.edu simbad sim basic?Ident 17 Aquarii&submit SIMBAD search 17 Aquarii accessed 2012 March 20 ref ra RA 21 22 56.25675 ref name SIMBAD dec DEC 09 19 09.5829 ref name SIMBAD 17 Aquarii is a spectroscopic binary star in the constellation Aquarius constellation Aquarius . Its apparent magnitude is 5.99. References reflist Stars of Aquarius Category Aquarius constellation Category Spectroscopic binaries Category M type stars Category Giant stars Category Flamsteed objects Aquarii, 17 binary star stub ca 17 Aquarii it 17 Aquarii tr 17 Aquarii ... more details
Algol variables or Algol type binaries are a class of eclipse eclipsing binary star s where the Orbital plane astronomy orbital plane of the stars are coincident with the line of sight from Earth. ref cite journal title A consideration of close binary systems in relation to light variation. journal Report of the South African Association for the Advancement of Science year 1903 volume 1 pages 110 111 accessdate 11 August 2010 ref When the cooler component passes in front of the hotter one, part of the latter s light is blocked, and the total brightness of the binary, as viewed from Earth , temporarily decreases. This is the primary minimum of the binary. Total brightness may also decrease, but less, when the hotter component passes in front of the cooler one this is the secondary minimum. The Frequency period , or time span between two primary minima, is very regular, being determined by the Orbital revolution revolution period of the binary, the time it takes for the two components to once orbit around each other. Most Algol variables are quite close binaries, and therefore their periods are short, typically a few days. The shortest known period is 0.1167 days 2 48 hours, HW Virginis the longest is 9892 days 27 years, epsilon Aurigae . Component stars of Algol binary systems have a sphere spherical , or slightly ellipsoidal shape. This distinguishes them from the so called beta Lyrae variable s and W Ursae Majoris variable s, where the two components are so close that gravitation al effects lead to serious deformations of both stars. Generally the amplitude s of the brightness variations are of the order of one Apparent magnitude magnitude , the largest variation known being 3.4 magnitudes V342 Aquilae . The components may have any stellar classification spectrum , though ... explained by John Goodricke in 1782. Many thousands of Algol binaries are now known the latest ... Category Eclipsing binaries Category Binary stars Category Variable stars ca Variable Algol ... more details
Orphan date February 2009 In the OpenSolaris world, a Blindingly Fast Upgrade BFU or Bonwick Faulkner Upgrade or Big F ing Upgrade , is a process used to upgrade a subset of a Solaris system s binaries using cpio archives instead of full software packages. ref name opensolaris cite web url http www.opensolaris.org os community on devref toc devref 5 title Installing and Testing ON accessdate 2007 10 10 date 2006 04 05 publisher Sun Microsystems, Inc. ref BFUs are not a recommended method for end users to upgrade their systems but the OpenSolaris developers and enthusiasts wanting the latest features on their machines use this as a fast way to upgrade the software on their machine. ref name opensolaris Notes and references Reflist Category Package management systems Category OpenSolaris Install software stub ... more details
Unreferenced stub date December 2009 In the study of asteroids, a contact binary is caused when two asteroids gravitate toward each other until they touch, forming an oddly shaped single body. Asteroids suspected of being contact binaries include the unusually elongated 624 Hektor and the wikt bilobate bilobated 216 Kleopatra and 4769 Castalia . 25143 Itokawa , recently photographed by the Hayabusa probe, also appears to be a contact binary which has resulted in an elongated, bent body. See also Rubble pile Binary system astronomy Asteroids DEFAULTSORT Contact Binary Asteroid Category Asteroids Astronomy stub zh ... more details
CPack is a packaging system for software distributions which is tightly integrated with CMake , but can function without it. It allows you to generate Linux RPM package RPM , Debian package deb and gzip distributions of both binaries and source code . Nullsoft Scriptable Install System NSIS files for Microsoft Windows Mac OS X packages See also EPM dn date January 2012 Nullsoft Scriptable Install System Inno Setup External links http www.cmake.org Wiki CMake Packaging With CPack Packaging With CPack Category Build automation ... more details
This is a partial list of known accretion powered pulsars , as of 1997. LMXB class wikitable Low Mass Binaries Spin Period sec Orbital Period days Companion Stellar Classification Harvard spectral classification MK Type GRO J1744 28 0.467 11.8 unknown 4U 1626 67 7.66 0.0289 KZ TrA low mass dwarf 4U 1728 247 GX 1 4 120 unknown V2116 Oph M6 III IMXB class wikitable Intermediate Mass Binaries Spin Period sec Orbital Period days Companion Stellar Classification Harvard spectral classification MK Type Hercules X 1 Her X 1 1.24 1.7 HZ Her A9 B HMXB class wikitable High Mass Binaries Spin Period sec Orbital Period days Companion Stellar Classification Harvard spectral classification MK Type SMC X 1 0.717 3.89 Sk 160 B0 I Centaurus X 3 Cen X 3 4.82 2.09 V779 Cen O6 8f RX J0648.1 4419 13.2 1.54 HD 49798 O6p LMC X 4 13.5 1.41 Sk Ph O7 III V OAO 1657 415 37.7 10.4 B0 6 Iab Vela X 1 283 8.96 HD 77581 B0.5 Ib 1E 1145.1 6141 297 unknown V830 Cen B2 Iae 4U 1907 09 438 8.38 B I 4U 1538 52 530 3.73 QV Nor B0 Iab GX 301 2 681 41.5 Way 977 BI.5 Ia BeXB class wikitable Transient Be star Binary Systems Spin Period sec Orbital Period days Companion Stellar Classification Harvard spectral classification MK Type A0538 67 0.069 16.7 B2 III IVe 4U 0115 63 3.61 24.3 V635 Cas Be V0332 53 4.37 34.2 BQ Cam Be 2S 1417 624 17.6 42.1 OBe EXO 2030 375 41.7 46.0 Be GRO J1008 57 93.5 248 Be A0535 26 105 110 HDE 245770 09.7 IIe GX 304 1 272 133 ? V850 Cen B2 Vne 4U 1145 619 292 187 Hen 715 BI Vne A1118 616 405 unknown He 3 640 O9.5 III Ve 4U 0352 309 835 unknown X Per O9 III Ve RX J0146.9 6121 1413 unknown LS I 61 235 B5 IIIe Expand list date February 2011 References reflist http adsabs.harvard.edu abs 1997ApJS..113..367B Observations of Accreting Pulsars , Bildsten, L., et al., 1997, Astrophysical Journal Supplement Series, 113 , p. 367 Category Pulsars List of X ray pulsars Category X ray binaries List of X ray pulsars Category X ray pulsars Category Lists of stars X ray pulsars var star stub sk Zozn ... more details
The Family D Alembert series is a set of science fiction novels by Stephen Goldin , the first of which was expanded from a novella by E E Doc Smith E. E. Doc Smith . Plot Jules and Yvette D Alembert are a brother and sister team of aerialists in the D Alembert family Circus of the Empire and also work as agents in SOTE, The Service of The Empire , the imperial intelligence agency. Series The series comprises the following books Imperial Stars 1976 Stranglers Moon 1976 The Clockwork Traitor 1976 Getaway World 1977 Appointment at Bloodstar , also known as The Bloodstar Conspiracy 1978 The Purity Plot 1978 Planet of Treachery 1981 Eclipsing Binaries 1983 The Omicron Invasion 1984 Revolt of the Galaxy 1985 Category Science fiction book series ... more details
In free and open source software , a Computer software software maintainer is usually one or more people who build source code into a Executable binary Software package installation package for Software deployment distribution , commit Patch computing patches , or organize code in a Codebase source repository . ref cite web url http www.linux.com feature 142765 title OLS Kernel documentation, and submitting kernel patches author David cdlu Graham publisher Linux.com date 2008 07 25 accessdate 2008 08 20 ref Maintainers often digital signature cryptographically sign binaries so that people can verify their authenticity. See also Software maintenance Software developer References reflist Category Software maintenance software eng stub de Maintainer fa fi Yll pit j fr Mainteneur nl Maintainer ... more details
bilateral Bulgarian Dutch Bulgaria Netherlands Bulgarian Dutch relations are foreign relations between Bulgaria and the Netherlands . Bulgaria has an embassy in The Hague . The Netherlands has an embassy in Sofia . Both countries are full members of NATO and of the European Union . See also Foreign relations of Bulgaria Foreign relations of the Netherlands External links http www.mfa.bg hague Bulgarian embassy The Hague http www.minbuza.nl binaries pdf reizen en landen betrekkingen met nederland bulgarije format .pdf Dutch Ministry of Foreign Affairs about relations with Bulgaria in Dutch only http www.mfa.nl sof en Dutch embassy Sofia Foreign relations of Bulgaria Foreign relations of the Netherlands Category Bilateral relations of Bulgaria Netherlands fixcategory Category Bilateral relations of the Netherlands foreignrelations stub ... more details
Bilateral Dutch Slovenian Netherlands Slovenia Dutch Slovenian relations are foreign relations between the Netherlands and Slovenia . Both countries established diplomatic relations on June 25, 1991. The Netherlands has an embassy in Ljubljana . Slovenia has an embassy in The Hague . Both countries are full members of NATO and of the European Union . See also Foreign relations of the Netherlands Foreign relations of Slovenia External links http www.minbuza.nl binaries pdf reizen en landen betrekkingen met nederland slovenie.pdf Dutch Ministry of Foreign Affairs about relations with Slovenia in Dutch only http slovenia.nlembassy.org homepage Dutch embassy in Ljubljana http hague.embassy.si index.php?id 29&L 1 Slovenian embassy in The Hague Foreign relations of the Netherlands Foreign relations of Slovenia Category Bilateral relations of the Netherlands S ovenia fixcategory Category Bilateral relations of Slovenia foreignrelations stub ... more details
Infobox Observatory name Beersel Hills Observatory background image caption organization code location Beersel , Belgium coords coords 50.7602 4.3036 display inline,title altitude weather established closed website http users.skynet.be bho index.htm users.skynet.be bho index.htm telescope1 name telescope1 type telescope2 name telescope2 type telescope3 name telescope3 type telescope4 name telescope4 type Beersel Hills Observatory is an amateur astronomy astronomical observatory . Founded in April 1998, it is located near Beersel , Belgium . It is primarily dedicated to the study of variable star s and visual double stars, including Delta Scuti , eclipsing binaries, and visual double stars. External links http users.skynet.be bho index.htm Beersel Hills Observatory Category Astronomical observatories in Belgium Category Buildings and structures in Flemish Brabant observatory stub ... more details
The GEMIX is a report, completed on September 30, 2009 and published on 9 October 2009, and commissioned by the Belgium Belgian Minister Paul Magnette . The complete title in French is Quel mix nerg tique id al pour la Belgique Analyse aux horizons 2020 et 2030 ? . The report had a lot of publicity mainly to its recommandation on nuclear power . The report was written by Dominique Woitrin, Marie Pierre Fauconnier, Danielle Devogelaer, Jacques Percebois, Luigi De Paoli, Jacques De Ruyck and Wolfgang Eichhammer. Luc Dufresne was president of the workgroup. See also Energy in Belgium Sources http economie.fgov.be fr binaries rapport gemix 2009 fr tcm326 76356.pdf The report Category Energy in Belgium ... more details
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