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

• Published in: Astronomische Nachrichten 2004-02, Vol.325 (2), p.100-103
• Main Authors: McDermid, R., Emsellem, E., Cappellari, M., Kuntschner, H., Bacon, R., Bureau, M., Copin, Y., Davies, R. L., Falcón-Barroso, J., Ferruit, P., Krajnović, D., Peletier, R.F., Shapiro, K., Wernli, F., de Zeeuw, P.T.
• Format: Article
• Language: English
• Subjects: Astrophysics; Cosmology and Extra-Galactic Astrophysics; galaxies: elliptical and lenticular; galaxies: individual (NGC2768; galaxies: individual (NGC2768, NGC3489, NGC4382); galaxies: kinematics and dynamics; galaxies: stellar content; NGC3489; NGC4382; Physics; Sciences of the Universe
• ISSN: 0004-6337; 1521-3994
• DOI: 10.1002/asna.200310184

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)