SIMBAD references

2011AJ....142..113W - Astron. J., 142, 113 (2011/October-0)

The candidate intermediate-mass black hole in the globular cluster M54.


Abstract (from CDS):

Ibata et al. reported evidence for density and kinematic cusps in the Galactic globular cluster M54, possibly due to the presence of a 9400 M black hole. Radiative signatures of accretion onto M54's candidate intermediate-mass black hole (IMBH) could bolster the case for its existence. Analysis of new Chandra and recent Hubble Space Telescope astrometry rules out the X-ray counterpart to the candidate IMBH suggested by Ibata et al. If an IMBH exists in M54, then it has an Eddington ratio of L(0.3-8 keV)/L(Edd) < 1.4x10–10, more similar to that of the candidate IMBH in M15 than that in G1. From new imaging with the NRAO Very Large Array, the luminosity of the candidate IMBH is L(8.5 GHz) < 3.6x1029 erg/s (3σ). Two background active galaxies discovered toward M54 could serve as probes of its intracluster medium.

Abstract Copyright:

Journal keyword(s): black hole physics - globular clusters: individual: M54 - radio continuum: general - X-rays: general

Nomenclature: Paragr. 2.3: [WGH2011] VLA N=2.

Status at CDS:  

CDS comments: Calibrator J1845-2852 is not in SIMBAD.

Simbad objects: 19

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