A Kinematic Study of the Nuclear Stellar Populations in Seyfert Galaxies

Astronomy and Astrophysics – Astrophysics

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Scientific paper

Recent studies in the optical and UV have detected circumnuclear starbursts in 40% of nearby Seyfert-2 galaxies; about half of the remaining 60% present a UV excess whose nature is not well known, mainly because of the limitations of the current stellar population analysis techniques in the optical and UV domains. A possible way to circumvent these difficulties is to use a determination of the mass-to-light (M/L) ratio, obtained with a combination of velocity dispersion measurements and photometric information. Dynamical information in AGN (particularly in type 2) is better determined from NIR spectroscopic data, where the stellar absorption features are less affected by the nuclear continuum dilution. In this work, we present preliminary results of a spectroscopic survey of more than 60 Seyfert nuclei (mainly Seyfert 2s), conducted at ESO/La Silla and at KPNO. For many of these objects we have complementary data, such as HST images, optical and (in some cases) UV spectroscopy. The long-slit spectroscopy for the purpose of this project was performed around the NIR Ca II triplet lines at 8498, 8542 and 8662Å. Here we describe the analysis steps taken so far, and present the first results concerning velocity dispersion measurements in nuclear regions. With these data we aim to investigate the ambiguous Seyfert 2 nuclei nature, thus contributing to a better understanding of the AGN-starburst connection.

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