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Title: SPATIALLY RESOLVED SPECTROSCOPY OF THE GLOBULAR CLUSTER RZ 2109 AND THE NATURE OF ITS BLACK HOLE

Journal Article · · Astrophysical Journal
;  [1];  [2];  [3]; ;  [4];  [5]; ;  [6];  [7]
  1. Department of Physics and Astronomy, Michigan State University, East Lansing, MI 48824 (United States)
  2. Eureka Scientific, Inc., 2452 Delmer Street, Suite 100 Oakland, CA 94602 (United States)
  3. School of Physics and Astronomy, University of Southampton, Southampton SO17 1BJ (United Kingdom)
  4. Department of Astronomy, Indiana University, Bloomington, IN 47405 (United States)
  5. Institute for Astronomy, University of Hawaii at Manoa, Honolulu, HI 96822 (United States)
  6. Department of Astronomy and Astrophysics, Pennsylvania State University, University Park, PA 16802 (United States)
  7. Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109 (United States)

We present optical Hubble Space Telescope/Space Telescope Imaging Spectrograph (HST/STIS) spectroscopy of RZ 2109, a globular cluster (GC) in the elliptical galaxy NGC 4472. This GC is notable for hosting an ultraluminous X-ray source as well as associated strong and broad [O III] {lambda}{lambda}4959, 5007 emission. We show that the HST/STIS spectroscopy spatially resolves the [O III] emission in RZ 2109. While we are unable to make a precise determination of the morphology of the emission-line nebula, the best-fitting models all require that the [O III] {lambda}5007 emission has a half-light radius in the range 3-7 pc. The extended nature of the [O III] {lambda}5007 emission is inconsistent with published models that invoke an intermediate-mass black hole origin. It is also inconsistent with the ionization of ejecta from a nova in the cluster. The spatial scale of the nebula could be produced via the photoionization of a strong wind driven from a stellar mass black hole accreting at roughly its Eddington rate.

OSTI ID:
22086361
Journal Information:
Astrophysical Journal, Vol. 759, Issue 2; Other Information: Country of input: International Atomic Energy Agency (IAEA); ISSN 0004-637X
Country of Publication:
United States
Language:
English