Abstract
We have recently completed a 64 night spectroscopic monitoring campaign at the Lick Observatory 3 m Shane telescope with the aim of measuring the masses of the black holes in 13 nearby (z<0.05) Seyfert 1 galaxies with expected masses in the range-106-107 M⊙. We present here the first results from this project-the mass of the central black hole in Arp 151. Strong variability throughout the campaign led to an exceptionally clean Hβ lag measurement in this object of 4.25+0.68-0.66 days in the observed frame. Coupled with the width of the Hβ emission line in the variable spectrum, we determine a black hole mass of (7.1 ± 1.2) × 106 M⊙, assuming the Onken et al. normalization for reverberation-based virial masses. We also find velocity-resolved lag information within the Hβ emission line which clearly shows infalling gas in the Hβ-emitting region. Further detailed analysis may lead to a full model of the geometry and kinematics of broad line region gas around the central black hole in Arp 151.
Original language | English (US) |
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Pages (from-to) | L21-L24 |
Journal | Astrophysical Journal |
Volume | 689 |
Issue number | 1 PART 2 |
DOIs | |
State | Published - 2008 |
All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics
- Space and Planetary Science
Keywords
- Galaxies: Individual (Arp 151)
- Galaxies: Nuclei
- Galaxies: Seyfert
- Galaxies: active