Sub-galactic clumps at a redshift of 2.39 and implications for galaxy formation

Details Sub-galactic clumps at a redshift of 2.39 and implications for galaxy formation Sub-galactic clumps at a redshift of 2.39 and implications for galaxy formation

Sep 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996natur.383...45p&link_type=abstract

Nature, Volume 383, Issue 6595, pp. 45-50 (1996).

Computer Science

132

Scientific paper

A large number of very faint, compact objects have been found at a redshift of 2.39 in optical images of the distant Universe. The objects appear to be star-forming spheroids smaller than the bulge of a spiral galaxy; they are much smaller and fainter than typical galaxies seen today. These objects may be part of a reservoir from which many of today's luminous galaxies were formed through repeated mergers.

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