Maps of BzK-15504

SINFONI maps of H-alphaline emission in BzK-15504, separated in 65 km/s bins of Doppler velocity (marked at the bottom left of each image) and centred on the systemic cosmological redshift of the galaxy (z=2.38). North is up and East is to the left, and a bar marks the angular scale of 0.5". The high resolution, spectrally resolved images show with exquisite clarity that star formation in this distant galaxy occurs in spectacular luminous complexes (bright spots) and that gas is funnelled at large rates into the nuclear region, forming a dense stellar bulge there. Over time, this system may transform into a compact, dense elliptical galaxy.

Crédit:

ESO

À propos de l'image

Identification:eso0631b
Type:Observation
Date de publication:17 août 2006
Communiqués de presse en rapport:eso0631
Taille:2508 x 1620 px

À propos de l'objet

Nom:BzK 15504
Type:Early Universe : Galaxy : Activity : AGN
Distance:z=2.38 (redshift)
Catégorie:Galaxies
Quasars and Black Holes

Image Formats

Grand JPEG
601,1 Kio
JPEG taille écran
140,2 Kio

Fonds d'écran

1024x768
191,4 Kio
1280x1024
284,5 Kio
1600x1200
376,2 Kio
1920x1200
406,3 Kio
2048x1536
552,1 Kio

Couleurs & filtres

DomaineTélescope
Infrarouge
H-alpha
Very Large Telescope
SINFONI