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A local baseline of the black hole mass scaling relations for active galaxies. III. The M{sub BH}–σ relation

Journal Article · · Astrophysical Journal
; ;  [1];  [2];  [3];  [4];  [5];  [6];  [7]
  1. Physics Department, California Polytechnic State University, San Luis Obispo, CA 93407 (United States)
  2. Department of Physics, University of California, Santa Barbara, CA 93106 (United States)
  3. Institute of Astronomy, Madingley Road, Cambridge CB3 0HA (United Kingdom)
  4. National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012 (China)
  5. Lawrence Berkeley National Laboratory, Berkeley, CA 94720 (United States)
  6. Department of Physics and Astronomy, University of California, Los Angeles, CA 90095 (United States)
  7. Department of Astronomy, Seoul National University (Korea, Republic of)

We create a baseline of the black hole (BH) mass (M{sub BH})—stellar-velocity dispersion (σ) relation for active galaxies, using a sample of 66 local (0.02

OSTI ID:
22882863
Journal Information:
Astrophysical Journal, Journal Name: Astrophysical Journal Journal Issue: 1 Vol. 809; ISSN ASJOAB; ISSN 0004-637X
Country of Publication:
United Kingdom
Language:
English