Michele Cappellari: Publications

The SAURON project - XIII. SAURON-GALEX study of early-type galaxies: the ultraviolet colour-magnitude relations and Fundamental Planes

(2009)

Authors:

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

The SAURON Project - XIV. No escape from V$_{\mathrm{esc}}$: a global and local parameter in early-type galaxy evolution

(2009)

Authors:

Nicholas Scott, Michele Cappellari, Roger L Davies, R Bacon, PT de Zeeuw, Eric Emsellem, Jesus Falcon-Barroso, Davor Krajnovic, Harald Kuntschner, Richard M McDermid, Reynier F Peletier, Antonio Pipino, Marc Sarzi, Remco CE van den Bosch, Glenn van de Ven, Eveline van Scherpenzeel

Stellar velocity profiles and line strengths out to four effective radii in the early-type galaxies NGC 3379 and NGC 821

(2009)

Authors:

A Weijmans, M Cappellari, R Bacon, PT de Zeeuw, E Emsellem, J Falcon-Barroso, H Kuntschner, RM McDermid, RCE van den Bosch, G van de Ven

A Shared Tully-Fisher Relation for Spiral and S0 Galaxies

(2009)

Authors:

Michael J Williams, Martin Bureau, Michele Cappellari

An H I view of the on-going assembly of early-type galaxies: Present and future observations

Proceedings of Science 89 (2009)

Authors:

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

Abstract:

We present a preliminary analysis of the H I properties of early-type galaxies in the ATLAS^3D sample. Using WSRT data for ~100 galaxies outside the Virgo cluster and data from the Alfalfa project for galaxies inside Virgo, we discuss the dependence of H I properties on environment. We detect H I in about half of the galaxies outside Virgo. For these systems, the H I morphology and kinematics change as a function of environment, going from regular, rotating systems around “isolated” galaxies to progressively more disturbed structures for galaxies with neighbours or in groups. In denser environment, inside Virgo, nearly none of the galaxies contains H I. We discuss future work in this field which will be enabled by next-generation, pre-SKA radio instruments. We present a simulated Apertif H I observation of an ATLAS^3D early-type galaxy, showing how its appearance and detection level vary as a function of redshift.

51��