A VERY LARGE ARRAY SEARCH FOR INTERMEDIATE-MASS BLACK HOLES IN GLOBULAR CLUSTERS IN M81

作者：Wrobel J M^*; Miller Jones J C A; Middleton M J

来源：Astronomical Journal, 2016, 152(1): 22.

DOI：10.3847/0004-6256/152/1/22

• black hole physics
• galaxies: individual (M81)
• galaxies: star clusters: individual (M81, ESO 243-49 HLX-1, M60-UCD1)
• radio continuum: general

Nantais et al. used the Hubble Space Telescope to localize probable globular clusters (GCs) in M81, a spiral galaxy at a distance of 3.63 Mpc. Theory predicts that GCs can host intermediate-mass black holes (IMBHs) with masses M-BH similar to 100-100,000 M-circle dot. Finding IMBHs in GCs could validate a formation channel for seed BHs in the early universe, bolster gravitational-wave predictions for space missions, and test scaling relations between stellar systems and the central BHs they host. We used the NRAO Karl G. Jansky Very Large Array to search for the radiative signatures of IMBH accretion from 206 probable GCs in a mosaic of M81. The observing wavelength was 5.5 cm, and the spatial resolution was 1.'' 5 (26.4 pc). None of the individual GCs are detected, nor are weighted-mean image stacks of the 206 GCs and the 49 massive GCs with stellar masses M-star greater than or similar to 200,000 M-circle dot. We apply a semiempirical model to predict the mass of an IMBH that, if undergoing accretion in the long-lived, hard X-ray state, is consistent with a given radio luminosity. The 3 sigma radio-luminosity upper limits correspond to IMBH masses of <(M-BH (all))over bar> < 42,000 M-circle dot for the all-cluster stack and <(M-BH (massive))over bar> < 51,000 M-circle dot for the massive-cluster stack. We also apply the empirical fundamental-plane relation to two X-ray-detected clusters, finding that their individual IMBH masses at 95% confidence are M-BH < 99,000 M-circle dot and M-BH < 15,000 M-circle dot. Finally, no analog of HLX-1, a strong IMBH candidate in an extragalactic star cluster, occurs in any individual GC in M81. This underscores the uniqueness or rarity of the HLX-1 phenomenon.

• 出版日期2016-7
• 单位国家自然科学基金委员会