Michele Cappellari: Publications

The SAURON project XVI: On the Sources of Ionisation for the Gas in Elliptical and Lenticular Galaxies

(2009)

Authors:

Marc Sarzi, Joseph C Shields, Kevin Schawinski, Hyunjin Jeong, Kristen Shapiro, Roland Bacon, Martin Bureau, Michele Cappellari, Roger L Davies, P Tim de Zeeuw, Eric Emsellem, Jesus Falcon-Barroso, Davor Krajnovic, Harald Kuntschner, Richard M McDermid, Reynier F Peletier, Remco CE van den Bosch, Glen van den Ven, Sukyoung K Yi

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Kinematic constraints on the stellar and dark matter content of spiral and S0 galaxies

(2009)

Authors:

Michael J Williams, Martin Bureau, Michele Cappellari

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Scaling relations in early-type galaxies from integral-field stellar kinematics

(2009)

Authors:

M Cappellari, N Scott, K Alatalo, L Blitz, M Bois, F Bournaud, M Bureau, RL Davies, TA Davis, PT de Zeeuw, E Emsellem, J Falcon-Barroso, S Khochfar, D Krajnovic, H Kuntschner, P-Y Lablanche, RM McDermid, R Morganti, T Naab, M Sarzi, P Serra, RCE van den Bosch, G van de Ven, A Weijmans, LM Young

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Determination of masses of the central black holes in NGC524 and NGC2549 using Laser Guide Star Adaptive Optics

(2009)

Authors:

Davor Krajnovic, Richard M McDermid, Michele Cappellari, Roger L Davies

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Stellar populations of early-type galaxies in the ATLAS^3D sample

AIP Conference Proceedings 1111 (2009) 111-114

Authors:

P Serra, RM McDermid, K Alatalo, L Blitz, M Bois, F Bournaud, M Bureau, M Cappellari, RL Davies, TA Davis, PT De Zeeuw, E Emsellem, J Falcón-Barroso, S Khochfar, D Krajnović, H Kuntschner, PY Lablanche, R Morganti, T Naab, M Sarzi, N Scott, RCE Van Den Bosch, G Van De Ven, A Weijmans, LM Young

Abstract:

ATLAS3D is a multi-wavelength, volume-limited survey of 263 morphologicallyselected early-type galaxies within a distance of 42 Mpc and complete to MK ≤ -21.5. Here we present the ATLAS3D project and our first results on the stellar populations of galaxies in the ATLAS3Dsample based on SAURON integral-field spectroscopy. We show relations between integrated line-strength indices and stellar velocity dispersion o in the range 55 ≤ Σ(km/s) ≤ 350. We derive simple-stellar-population-equivalent age, metallicity and α/Fe abundance ratio and discuss their relation to stellar velocity dispersion, environment and galaxy internal kinematics. These preliminary results indicate that slow rotators tend to be older and have less variation in age than fast rotators. We also find that galaxies in lower density environments are on average younger than those in denser environments, as found by other authors. © 2009 American Institute of Physics.

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Michele Cappellari

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The SAURON project XVI: On the Sources of Ionisation for the Gas in Elliptical and Lenticular Galaxies

Authors:

Kinematic constraints on the stellar and dark matter content of spiral and S0 galaxies

Authors:

Scaling relations in early-type galaxies from integral-field stellar kinematics

Authors:

Determination of masses of the central black holes in NGC524 and NGC2549 using Laser Guide Star Adaptive Optics

Authors:

Stellar populations of early-type galaxies in the ATLAS^3D sample

Authors:

Abstract:

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The SAURON project XVI: On the Sources of Ionisation for the Gas in Elliptical and Lenticular Galaxies

Authors:

Kinematic constraints on the stellar and dark matter content of spiral and S0 galaxies

Authors:

Scaling relations in early-type galaxies from integral-field stellar kinematics

Authors:

Determination of masses of the central black holes in NGC524 and NGC2549 using Laser Guide Star Adaptive Optics

Authors:

Stellar populations of early-type galaxies in the ATLAS3D sample

Authors:

Abstract:

Stellar populations of early-type galaxies in the ATLAS^3D sample