FIRST RESULTS FROM THE LICK AGN MONITORING PROJECT: THE MASS OF THE BLACK HOLE IN ARP 151

被引:68
作者
Bentz, Misty C. [1 ]
Walsh, Jonelle L. [1 ]
Barth, Aaron J. [1 ]
Baliber, Nairn [2 ,3 ]
Bennert, Nicola [2 ,4 ]
Canalizo, Gabriela [4 ,5 ]
Filippenko, Alexei V. [6 ]
Ganeshalingam, Mohan [6 ]
Gates, Elinor L. [7 ]
Greene, Jenny E. [8 ]
Hidas, Marton G. [2 ,3 ]
Hiner, Kyle D. [4 ,5 ]
Lee, Nicholas [6 ]
Li, Weidong [6 ]
Malkan, Matthew A. [9 ]
Minezaki, Takeo [10 ]
Serduke, Frank J. D. [6 ]
Shiode, Joshua H. [6 ]
Silverman, Jeffrey M. [6 ]
Steele, Thea N. [6 ]
Stern, Daniel [11 ]
Street, Rachel A. [2 ,3 ]
Thornton, Carol E. [1 ]
Treu, Tommaso [2 ]
Wang, Xiaofeng [6 ,12 ,13 ]
Woo, Jong-Hak [2 ,9 ]
Yoshii, Yuzuru [10 ,14 ]
机构
[1] Univ Calif Irvine, Dept Phys & Astron, Irvine, CA 92697 USA
[2] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA
[3] Las Cumbres Observ Global Telescope, Goleta, CA 93117 USA
[4] Univ Calif Riverside, Inst Geophys & Planetary Phys, Riverside, CA 92521 USA
[5] Univ Calif Riverside, Dept Phys & Astron, Riverside, CA 92521 USA
[6] Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA
[7] Lick Observ, Mt Hamilton, CA 95140 USA
[8] Princeton Univ Observ, Princeton, NJ 08544 USA
[9] Univ Calif Los Angeles, Dept Phys & Astron, Los Angeles, CA 90024 USA
[10] Univ Tokyo, Sch Sci, Inst Astron, Tokyo 1810015, Japan
[11] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
[12] Tsinghua Univ, Dept Phys, Beijing 100084, Peoples R China
[13] Tsinghua Univ, Tsinghua Ctr Astrophys THCA, Beijing 100084, Peoples R China
[14] Univ Tokyo, Sch Sci, Res Ctr Early Univ, Tokyo 1130033, Japan
来源
ASTROPHYSICAL JOURNAL LETTERS | 2008年 / 689卷 / 01期
关键词
galaxies: active; galaxies: individual (Arp 151); galaxies: nuclei; galaxies: Seyfert;
D O I
10.1086/595719
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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 with expected masses in the range similar to 10(6)-10(7) M(circle dot). 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 H beta lag measurement in this object of 4.25(-0.66)(+0.68) days in the observed frame. Coupled with the width of the H beta emission line in the variable spectrum, we determine a black hole mass of (7.1 +/- 1.2) x 10(6) M(circle dot), assuming the Onken et al. normalization for reverberation-based virial masses. We also find velocity-resolved lag information within the H beta emission line which clearly shows infalling gas in the H beta-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.
引用
收藏
页码:L21 / L24
页数:4
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