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Super massive black holes in spiral galaxies: HST/STIS observations for 3 new objects

L. Coccato·E. Dalla Bonta'·M. Sarzi·A. Pizzella·E. M. Corsini·F. Bertola
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Abstract

We present long-slit HST/STIS measurements of the ionized-gas kinematics in the nucleus of three disk galaxies, namely NGC 2179, NGC 4343, NGC 4435. The sample galaxies have been selected on the basis of their ground-based spectroscopy, for displaying a strong central velocity gradient for the ionized gas, which is consistent with the presence of a circum nuclear keplerian disk (CNKD, Bertola et al. 1998; Funes et al. 2002) rotating around a super massive black hole (SMBH). For each target galaxy we obtained the H_alpha and [NII] 6583 AA kinematics along the major axis and two 0"25 parallel offset positions. Out of three objects only NGC 4435 turned out to have a disk of ionized gas in regular motion and a regular dust-lane morphology. Preliminary modeling indicates a SMBH mass one order of magnitude lower than the one expected from the M-sigma relation for galaxies (Ferrarese & Merritt 2000; Gebhardt et al. 2000).

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L. Coccato, E. Dalla Bonta', M. Sarzi, A. Pizzella, E. M. Corsini, F. Bertola. 2004-04-29. Super massive black holes in spiral galaxies: HST/STIS observations for 3 new objects. https://doi.org/10.1017/s1743921304001553

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