TY - JOUR
T1 - Fast and slow rotators
T2 - The build-up of the red sequence
AU - Emsellem, Eric
AU - Cappellari, Michele
AU - Krajnović, Davor
AU - Van De Ven, Glenn
AU - Bacon, R.
AU - Bureau, M.
AU - Davies, Roger L.
AU - De Zeeuw, P. T.
AU - Falcón-Barroso, Jesús
AU - Kuntschner, Harald
AU - McDermid, Richard M.
AU - Peletier, Reynier F.
AU - Sarzi, Marc
AU - Van Den Bosch, Remco C.E.
PY - 2007/7
Y1 - 2007/7
N2 - Using the unique dataset obtained within the course of the SAURON project, a radically new view of the structure, dynamics and stellar populations of early-type galaxies has emerged. We show that galaxies come in two broad flavours (slow and fast rotators), depending on whether or not they exhibit clear large-scale rotation, as indicated via a robust measure of the specific angular momentum of baryons. This property is also linked with other physical characteristics of early-type galaxies, such as: the presence of dynamically decoupled cores, orbital structure and anisotropy, stellar populations and dark matter content. I here report on the observed link between this baryonic angular momentum and a mass sequence, and how this uniquely relates to the building of the red sequence via dissipative/dissipationless mergers and secular evolution.
AB - Using the unique dataset obtained within the course of the SAURON project, a radically new view of the structure, dynamics and stellar populations of early-type galaxies has emerged. We show that galaxies come in two broad flavours (slow and fast rotators), depending on whether or not they exhibit clear large-scale rotation, as indicated via a robust measure of the specific angular momentum of baryons. This property is also linked with other physical characteristics of early-type galaxies, such as: the presence of dynamically decoupled cores, orbital structure and anisotropy, stellar populations and dark matter content. I here report on the observed link between this baryonic angular momentum and a mass sequence, and how this uniquely relates to the building of the red sequence via dissipative/dissipationless mergers and secular evolution.
KW - CD
KW - Galaxies: elliptical and lenticular
KW - Galaxies: evolution
KW - Galaxies: stellar dynamics
UR - http://www.scopus.com/inward/record.url?scp=46749105646&partnerID=8YFLogxK
U2 - 10.1017/S1743921308017158
DO - 10.1017/S1743921308017158
M3 - Article
AN - SCOPUS:46749105646
VL - 3
SP - 11
EP - 14
JO - Proceedings of the International Astronomical Union
JF - Proceedings of the International Astronomical Union
SN - 1743-9213
IS - S245
ER -