2004MNRAS.351.1049M

Query : 2004MNRAS.351.1049M

2004MNRAS.351.1049M - Mon. Not. R. Astron. Soc., 351, 1049-1053 (2004/July-1)

Radio emission as a test of the existence of intermediate-mass black holes in globular clusters and dwarf spheroidal galaxies.

MACCARONE T.J.

Abstract (from CDS):

We take the established relation between black hole mass, X-ray luminosity and radio luminosity and show that intermediate-mass black holes (IMBHs), such as those predicted to exist at the centres of globular clusters (GCs), will be easily identifiable objects in deep radio observations. We show that the radio observations will be far more sensitive than any possible X-ray observations. We also discuss the likely optical photometric and spectroscopic appearance of such systems in the event that radio detections are made.

Abstract Copyright: 2004 RAS

Journal keyword(s): accretion, accretion discs - black hole physics - globular clusters: general - globular clusters: individual: Omega Cen - radio continuum: general

Simbad objects: 17

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Number of rows : 17
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 NGC 104 GlC 00 24 05.359 -72 04 53.20     4.09     ~ 4158 0
2 NGC 2808 GlC 09 12 03.10 -64 51 48.6           ~ 1540 0
3 NGC 5139 GlC 13 26 47.28 -47 28 46.1           ~ 3677 0
4 M 5 GlC 15 18 33.22 +02 04 51.7     5.95     ~ 2095 0
5 M 13 GlC 16 41 41.634 +36 27 40.75     5.8     ~ 2291 0
6 M 62 GlC 17 01 12.60 -30 06 44.5           ~ 668 0
7 M 19 GlC 17 02 37.69 -26 16 04.6   8.45 5.57     ~ 406 1
8 NGC 6388 GlC 17 36 17.461 -44 44 08.34           ~ 988 1
9 M 14 GlC 17 37 36.15 -03 14 45.3   9.55 5.73     ~ 420 0
10 NGC 6440 GlC 17 48 52.67 -20 21 34.5           ~ 592 0
11 NGC 6441 GlC 17 50 13.06 -37 03 05.2           ~ 940 0
12 M 28 GlC 18 24 32.89 -24 52 11.4           ~ 821 0
13 M 22 GlC 18 36 23.94 -23 54 17.1           ~ 1459 0
14 M 54 GlC 18 55 03.33 -30 28 47.5           ~ 1164 0
15 NGC 6752 GlC 19 10 52.11 -59 59 04.4           ~ 2121 0
16 PSR J1910-5959A Psr 19 11 42.7562 -59 58 26.900 22.02 22.13 22.03     DA5 99 1
17 M 15 GlC 21 29 58.33 +12 10 01.2           ~ 3274 0

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