The extreme synchronicity of stellar ages of red galaxies in the JKCS041 cluster at z=2.2

Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

A&A Letters, in press, english-revised version

Scientific paper

Above redshift z ~ 1.4, we known little or nothing about the stellar ages of red galaxies in clusters, yet at these high redshifts important changes are predicted by current renditions of galaxy formation models embedded in the standard hierarchical paradigm of structure formation. Red-sequence galaxies in the cluster JKCS041 at z=2.2 show a tight distribution in colour that indicates a star formation history that is highly synchronized across galaxies. Specifically, we measure a spread in stellar age of 160+/-30 Myr, in marked disagreement with the current understanding of how massive red galaxies form in clusters, i.e. if they are produced somewhat stochastically in merging episodes that sometimes involve gas, hence star formation. The existence of a tight distribution in colour when the universe was at one quarter of its current age implies that mechanisms that have not yet been implemented in current galaxy formation scenarios long ago began to shape the star formation history of red cluster galaxies.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

The extreme synchronicity of stellar ages of red galaxies in the JKCS041 cluster at z=2.2 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The extreme synchronicity of stellar ages of red galaxies in the JKCS041 cluster at z=2.2, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The extreme synchronicity of stellar ages of red galaxies in the JKCS041 cluster at z=2.2 will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-48551

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.