Matches in DBpedia 2016-04 for { <http://dbpedia.org/resource/Be/X-ray_binary> ?p ?o }
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- X-ray_binary abstract "Be/X-ray binaries (BeXRBs) 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-rays is seen.".
- X-ray_binary wikiPageID "211371".
- X-ray_binary wikiPageLength "2375".
- X-ray_binary wikiPageOutDegree "16".
- X-ray_binary wikiPageRevisionID "683623028".
- X-ray_binary wikiPageWikiLink Category:Be_stars.
- X-ray_binary wikiPageWikiLink Category:Binary_stars.
- X-ray_binary wikiPageWikiLink Category:X-ray_binaries.
- X-ray_binary wikiPageWikiLink Circinus_X-1.
- X-ray_binary wikiPageWikiLink Cygnus_X-3.
- X-ray_binary wikiPageWikiLink KT_(energy).
- X-ray_binary wikiPageWikiLink Karl_G._Jansky_Very_Large_Array.
- X-ray_binary wikiPageWikiLink LS_I_+61_303.
- X-ray_binary wikiPageWikiLink Neutron_star.
- X-ray_binary wikiPageWikiLink ROSAT.
- X-ray_binary wikiPageWikiLink SS_433.
- X-ray_binary wikiPageWikiLink Stellar_classification.
- X-ray_binary wikiPageWikiLink Stellar_wind.
- X-ray_binary wikiPageWikiLink Watt.
- X-ray_binary wikiPageWikiLink X-ray.
- X-ray_binary wikiPageWikiLink X-ray_binary.
- X-ray_binary wikiPageWikiLinkText "Be/X-ray binary".
- X-ray_binary wikiPageUsesTemplate Template:Neutron_star.
- X-ray_binary wikiPageUsesTemplate Template:Refimprove.
- X-ray_binary wikiPageUsesTemplate Template:Reflist.
- X-ray_binary wikiPageUsesTemplate Template:Star-system-stub.
- X-ray_binary subject Category:Be_stars.
- X-ray_binary subject Category:Binary_stars.
- X-ray_binary subject Category:X-ray_binaries.
- X-ray_binary hypernym Binaries.
- X-ray_binary comment "Be/X-ray binaries (BeXRBs) 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-rays is seen.".
- X-ray_binary label "Be/X-ray binary".
- X-ray_binary sameAs Q4875616.
- X-ray_binary sameAs Binário_emissor_de_raio_X_Be.
- X-ray_binary sameAs m.01d_8d.
- X-ray_binary sameAs Q4875616.
- X-ray_binary sameAs Be_X射線聯星.
- X-ray_binary wasDerivedFrom X-ray_binary?oldid=683623028.
- X-ray_binary isPrimaryTopicOf X-ray_binary.