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20 April 2024
 
  » arxiv » astro-ph/0512304

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Late-type galaxies observed with SAURON. Two-dimensional stellar and emission-line kinematics of 18 spirals
K. Ganda ; J. Falcón-Barroso ; R.F. Peletier ; M. Cappellari ; E. Emsellem ; R.M. McDermid ; P.T. de Zeeuw ; C.M. Carollo ;
Date 12 Dec 2005
Journal Mon.Not.Roy.Astron.Soc. 367 (2006) 46-78
AbstractWe present the stellar and gas kinematics of a sample of 18 nearby late-type spiral galaxies (Hubble types ranging from Sb to Sd), observed with the integral-field spectrograph SAURON at the 4.2-m William Herschel Telescope. SAURON covers the spectral range 4800-5380 A, allowing us to measure the Hbeta, Fe, Mgb absorption features and the emission in the Hbeta line and the [OIII], and [NI] doublets over a 33x41 arcsec field of view. The maps cover the nuclear region of these late-type galaxies and in all cases include the entire bulge. In many cases the stellar kinematics suggests the presence of a cold inner region, as visible from a central drop in the stellar velocity dispersion. The ionised gas is almost ubiquitous and behaves in a complicated fashion: the gas velocity fields often display more features than the stellar ones, including wiggles in the zero-velocity lines, irregular distributions, ring-like structures. The line ratio [OIII]/Hbeta often takes on low values over most of the field, probably indicating a wide-spread star formation.
Source arXiv, astro-ph/0512304
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