Äîêóìåíò âçÿò èç êýøà ïîèñêîâîé ìàøèíû. Àäðåñ îðèãèíàëüíîãî äîêóìåíòà : http://www.atnf.csiro.au/research/conferences/2013/gzo/abstracts/a66.html
Äàòà èçìåíåíèÿ: Mon Apr 11 10:55:42 2016
Äàòà èíäåêñèðîâàíèÿ: Mon Apr 11 21:50:22 2016
Êîäèðîâêà:
Ïîèñêîâûå ñëîâà: ï ï ï ï ï ï ï ï ï ï ï ï ï ï ï ï ï ï ï ï ï ï ï ï ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï
Evolutionary Paths in Galaxy Morphology

Morphological Transformation of Red Sequence Galaxies in High Redshift Galaxy Clusters

Pierluigi Cerulo (Swinburne University of Technology)

I present the results of a detailed analysis of the morphological properties of red sequence galaxies in a X-ray detected cluster at redshift z=0.98. Overall, the red sequence is dominated by elliptical and S0 galaxies. The fraction of S0s decreases at faint luminosities, where disc-dominated systems tend to become more frequent. From the comparison with a sample of local galaxy clusters, I discuss possible scenarios for the evolution of galaxies of different morphologies. I finally show the ongoing application of the analysis developed for this cluster to a sample of galaxy clusters at 0.8

á© 2013 Julie Banfield | Template design by andreasviklund.com and Tor Lundberg

Projects
Public