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・ Virgo (constellation)
・ Virgo (moth)
・ Virgo (software)
・ Virgo (surname)
・ Virgo Blaktro and the Movie Disco
・ Virgo Cluster
・ Virgo Consortium
・ Virgo Fidelis Convent Senior School
・ Virgo interferometer
・ Virgo Stellar Stream
・ Virgo Supercluster
・ Virgo Vibes
・ Virgo Williams
・ Virgocentric flow
・ Virgohamna
VIRGOHI21
・ Virgolândia
・ Virgos Merlot
・ Virgularia
・ Virgulariidae
・ Virgílio Lopes
・ Virgílio Mendes
・ Virgínia
・ Viria Sugar Mill
・ Virial coefficient
・ Virial expansion
・ Virial mass
・ Virial stress
・ Virial theorem
・ Viriat


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VIRGOHI21 : ウィキペディア英語版
VIRGOHI21

VIRGOHI21 is an extended region of neutral hydrogen (HI) in the Virgo cluster discovered in 2005. Analysis of its internal motion indicates that it may contain a large amount of dark matter, as much as a small galaxy. Since VIRGOHI21 apparently contains no stars, this would make it one of the first detected dark galaxies. Skeptics of this interpretation argue that VIRGOHI21 is simply a tidal tail of the nearby galaxy NGC 4254.
==Observational properties==
VIRGOHI21 was detected through radio telescope observations of its neutral hydrogen 21 cm emissions. The detected hydrogen has a mass of about 100 million solar masses and is about 50 million light-years away.〔(【引用サイトリンク】title=New evidence for a Dark Matter Galaxy )〕 By analyzing the Doppler shift of the emissions, astronomers determined that the gas has a high velocity-profile width; that is, different parts of the cloud are moving at high speed relative to other parts. Follow-up Hubble space telescope deep observations of the region have detected very few stars (a few hundred).

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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