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A black-hole mass measurement from molecular gas kinematics in NGC4526

Author

Listed:
  • Timothy A. Davis

    (European Southern Observatory, Karl-Schwarzschild-Strasse 2, 85748 Garching-bei-München, Germany)

  • Martin Bureau

    (University of Oxford, Denys Wilkinson Building, Keble Road, Oxford OX1 3RH, UK)

  • Michele Cappellari

    (University of Oxford, Denys Wilkinson Building, Keble Road, Oxford OX1 3RH, UK)

  • Marc Sarzi

    (Centre for Astrophysics Research, University of Hertfordshire, Hatfield, Herts AL1 9AB, UK)

  • Leo Blitz

    (University of California)

Abstract

In this study a supermassive black-hole mass is measured by tracing the motions of molecular gas clouds swirling around it, a technique that promises to allow measurements of black-hole mass in many more galaxies of all types than previously possible.

Suggested Citation

  • Timothy A. Davis & Martin Bureau & Michele Cappellari & Marc Sarzi & Leo Blitz, 2013. "A black-hole mass measurement from molecular gas kinematics in NGC4526," Nature, Nature, vol. 494(7437), pages 328-330, February.
    • Handle: RePEc:nat:nature:v:494:y:2013:i:7437:d:10.1038_nature11819
    DOI: 10.1038/nature11819
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