X-ray background
The observed X-ray background is thought to result from, at the "soft" end (below 0.3 keV), galactic X-ray emission, the "galactic" X-ray background, and, at the "hard" end (above 0.3keV), from a combination of many unresolved X-ray sources outside of the Milky Way, the "cosmic" X-ray background (CXB). The galactic X-ray background is produced largely by emission from hot gas in the Local Bubble within 100 parsecs of the Sun.
Wikipage disambiguates
Wikipage redirect
Andrew FabianAstrophysical X-ray sourceBackgroundBradley C. EdwardsBrian J. BoyleChandra Deep Field SouthCosmic X-ray backgroundCosmic backgroundCosmic background radiationCosmic infrared backgroundDiffuse extragalactic background radiationIndex of physics articles (X)Index of radio propagation articlesList of space telescopesPaschen's lawPlasma cosmologySkylab_3X-ray astronomyX-ray background radiationX-ray source
Link from a Wikipage to another Wikipage
primaryTopic
X-ray background
The observed X-ray background is thought to result from, at the "soft" end (below 0.3 keV), galactic X-ray emission, the "galactic" X-ray background, and, at the "hard" end (above 0.3keV), from a combination of many unresolved X-ray sources outside of the Milky Way, the "cosmic" X-ray background (CXB). The galactic X-ray background is produced largely by emission from hot gas in the Local Bubble within 100 parsecs of the Sun.
has abstract
Le fond diffus de rayons X (en ...... yons X (mous, moyens ou durs).
@fr
Sehr früh in der Geschichte de ...... Energien steht dies noch aus.
@de
The observed X-ray background ...... active galactic nuclei (AGN).
@en
Tło rentgenowskie – promieniow ...... Chandra, XMM-Newton, INTEGRAL.
@pl
宇宙X線背景放射 (cosmic X-ray backgro ...... の85%以上が点源からの放射の寄せ集めであることが判明した。
@ja
Link from a Wikipage to an external page
Wikipage page ID
page length (characters) of wiki page
Wikipage revision ID
932,624,015
Link from a Wikipage to another Wikipage
wikiPageUsesTemplate
comment
Le fond diffus de rayons X (en ...... ources près de la Voie lactée.
@fr
Sehr früh in der Geschichte de ...... der darin enthaltenen Sterne.
@de
The observed X-ray background ...... within 100 parsecs of the Sun.
@en
Tło rentgenowskie – promieniow ...... inne, nierozróżnialne źródła.
@pl
宇宙X線背景放射 (cosmic X-ray backgro ...... の85%以上が点源からの放射の寄せ集めであることが判明した。
@ja
label
Fond diffus de rayons X
@fr
Röntgenhintergrund
@de
Tło rentgenowskie
@pl
X-ray background
@en
宇宙X線背景放射
@ja