Emission of the galaxy BzK-15504

H-alpha line emission of the galaxy BzK-15504, at cosmological redshift of 2.38, corresponding to a time of 3 billion years after the Big Bang. The colours show whether the ionised gas is moving away from us (red), toward us (blue) or is stationary (green), relative to the overall rest frame of the galaxy. These data, obtained with SINFONI and adaptive optics (resulting in a resolution of 0.15", or 4,000 light years at the distance of the galaxy), show for the first time very clearly the gas motions in such a distant galaxy in the Early Universe. The galaxy appears to be a disc, like our Milky Way, and rotates at 230 km/s about the yellow axis, which is centred on the nucleus of the galaxy (white cross).

Kilde:

ESO

Om bildet

ID:eso0631a
Type:Observasjon
Publiseringsdato:17. august 2006
Relaterte pressemeldinger:eso0631
Størrelse:2358 x 2598 px

Om objektet

Navn:BzK 15504
Type:Early Universe : Galaxy : Activity : AGN
Avstand:z=2.38 (rødforskyvning)
Kategori:Galaxies

Bildeformater

Stor JPEG
384,2 KB
Medium JPEG
121,3 KB

Skrivebordsbakgrunner

1024x768
111,6 KB
1280x1024
149,2 KB
1600x1200
188,3 KB
1920x1200
206,7 KB
2048x1536
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Farger og filtre

BåndTeleskop
Infrarødt
H-alpha
Very Large Telescope
SINFONI

 

Se også