TY - JOUR
T1 - The build-up of the colour-magnitude relation
AU - Tanaka, Masayuki
AU - Kodama, Tadayuki
PY - 2006/8
Y1 - 2006/8
N2 - We discuss the build-up of the colour-magnitude relation. The colour-magnitude relation first appears at the bright end and the faint end appears later. Interestingly, the build-up of colour-magnitude relation is delayed in low density environments. We suggest that galaxies follow the environment-dependent down-sizing evolution.
AB - We discuss the build-up of the colour-magnitude relation. The colour-magnitude relation first appears at the bright end and the faint end appears later. Interestingly, the build-up of colour-magnitude relation is delayed in low density environments. We suggest that galaxies follow the environment-dependent down-sizing evolution.
KW - Galaxies: clusters: general
KW - Galaxies: evolution
KW - Galaxies: fundamental parameters
UR - http://www.scopus.com/inward/record.url?scp=36949020646&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=36949020646&partnerID=8YFLogxK
U2 - 10.1017/S1743921306005734
DO - 10.1017/S1743921306005734
M3 - Article
AN - SCOPUS:36949020646
SN - 1743-9213
VL - 2
SP - 141
JO - Proceedings of the International Astronomical Union
JF - Proceedings of the International Astronomical Union
IS - S235
ER -
