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OASIS high‐resolution integral field spectroscopy of the SAURON ellipticals and lenticulars

2004; Wiley; Volume: 325; Issue: 2 Linguagem: Inglês

10.1002/asna.200310184

1521-3994

Richard M. McDermid, Éric Emsellem, Michele Cappellari, H. Kuntschner, Roland Bacon, Martin Bureau, Y. Copin, R. L. Davies, J. Falcón‐Barroso, Pierre Ferruit, D. Krajnović, R. F. Peletier, Kristen L. Shapiro, F. Wernli, P. T. de Zeeuw,

Astronomy and Astrophysical Research

Abstract We present a summary of high‐spatial resolution follow‐up observations of the elliptical (E) and lenticular (S0) galaxies in the SAURON survey using the OASIS integral field spectrograph. The OASIS observations explore the central 8″ × 10″ regions of these galaxies using a spatial sampling four times higher than SAURON, often revealing previously undiscovered features. Around 75% (31/48) of the SAURON E/S0s with central velocity dispersion ≳ 120 km s −1 were observed with OASIS, covering well the original SAURON representative sample.We present here an overview of this follow‐up survey, and some preliminary results on individual objects, including a previously unreported counter‐rotating core in NGC4382; the decoupled stellar and gas velocity fields of NGC2768; and the strong age gradient towards the centre of NGC3489. (© 2004 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)