Astrophysical X-ray source
Astrophysical X-ray sources are astronomical objects with physical properties which result in the emission of X-rays. There are a number of types of astrophysical objects which emit X-rays, from galaxy clusters, through black holes in active galactic nuclei (AGN) to galactic objects such as supernova remnants, stars, and binary stars containing a white dwarf (cataclysmic variable stars and super soft X-ray sources), neutron star or black hole (X-ray binaries). Some solar system bodies emit X-rays, the most notable being the Moon, although most of the X-ray brightness of the Moon arises from reflected solar X-rays. A combination of many unresolved X-ray sources is thought to produce the observed X-ray background. The X-ray continuum can arise from bremsstrahlung, either magnetic or ordinary
known for
Wikipage disambiguates
61 Ursae MajorisA Sky Full of GhostsAgata RóżańskaAmerican Astronomical Society 215th meetingApep (star system)Arp 147Astronomical X-ray sourceAstronomical X-ray sourcesAstronomical radio sourceAstronomyAstrophysical X-ray sourceC. Bruce TarterCalvera (X-ray source)Celestial X-ray sourceCoronal radiative lossesCosmic dustCosmos:_A_Spacetime_OdysseyCrab (unit)Cygnus X-1Cygnus X-3Diffuse X-ray backgroundExoplanetHerbert GurskyHistory of X-ray astronomyHolmberg IIIXPEIndex of physics articles (A)Jean SwankJuly–September 2020 in scienceList of plasma physics articlesList of the most distant astronomical objectsLockman HoleM60-UCD1MS 0735.6+7421Markarian 177Messier 15Messier 62NGC 5204NGC 5774
Link from a Wikipage to another Wikipage
primaryTopic
Astrophysical X-ray source
Astrophysical X-ray sources are astronomical objects with physical properties which result in the emission of X-rays. There are a number of types of astrophysical objects which emit X-rays, from galaxy clusters, through black holes in active galactic nuclei (AGN) to galactic objects such as supernova remnants, stars, and binary stars containing a white dwarf (cataclysmic variable stars and super soft X-ray sources), neutron star or black hole (X-ray binaries). Some solar system bodies emit X-rays, the most notable being the Moon, although most of the X-ray brightness of the Moon arises from reflected solar X-rays. A combination of many unresolved X-ray sources is thought to produce the observed X-ray background. The X-ray continuum can arise from bremsstrahlung, either magnetic or ordinary
has abstract
Als Röntgenquelle bezeichnet m ...... nur im Röntgenbereich zeigen.
@de
Astrophysical X-ray sources ar ...... owever long or brief a period.
@en
Les sources astrophysiques de ...... à un nuage coronal[pas clair].
@fr
São objetos astronômicos com p ...... aco negro (binário de raio X).
@pt
Źródło rentgenowskie – obiekt ...... y: Cygnus X-1, Scorpius X-1, .
@pl
Рентге́нівські джере́ла — астр ...... слабких джерел LX < 2×10-7 L☉.
@uk
Wikipage page ID
25.101.402
page length (characters) of wiki page
Wikipage revision ID
1.022.350.941
Link from a Wikipage to another Wikipage
wikiPageUsesTemplate
hypernym
comment
Als Röntgenquelle bezeichnet m ...... nur im Röntgenbereich zeigen.
@de
Astrophysical X-ray sources ar ...... g, either magnetic or ordinary
@en
Les sources astrophysiques de ...... ayonnement solaire sa surface.
@fr
São objetos astronômicos com p ...... aco negro (binário de raio X).
@pt
Źródło rentgenowskie – obiekt ...... y: Cygnus X-1, Scorpius X-1, .
@pl
Рентге́нівські джере́ла — астр ...... слабких джерел LX < 2×10-7 L☉.
@uk
label
Astrophysical X-ray source
@en
Fonte de raios X
@pt
Röntgenquelle (Astronomie)
@de
Source astrophysique de rayons X
@fr
Źródło rentgenowskie
@pl
Рентгенівські джерела
@uk