POSSIBLE EVIDENCE AGAINST A MASSIVE BLACK-HOLE AT THE GALACTIC-CENTER

Citation
A. Goldwurm et al., POSSIBLE EVIDENCE AGAINST A MASSIVE BLACK-HOLE AT THE GALACTIC-CENTER, Nature, 371(6498), 1994, pp. 589-591
Citations number
27
Categorie Soggetti
Multidisciplinary Sciences
Journal title
NatureACNP
ISSN journal
00280836
Volume
371
Issue
6498
Year of publication
1994
Pages
589 - 591
Database
ISI
SICI code
0028-0836(1994)371:6498<589:PEAAMB>2.0.ZU;2-M
Abstract
THE centre of our Galaxy is known to contain a large condensation of m ass(1), and it has been suggested that a massive black hole (of severa l million solar masses) is located there. Massive black holes have bee n proposed to explain active galactic nuclei, and if the Galactic Cent re is a less-powerful version of such sources it should radiate X-rays and gamma-rays(1). But although earlier observations(2-6) have shown that the region does emit X-rays and gamma-rays, the true centre, corr esponding to the object Sagittarius A, does not emit strongly at leas t up to energies of 30 keV (refs 4-6). Whether Sgr A emits radiation at higher energies, however, was not resolved. Here we present the res ults of a deep imaging survey of the Galactic Centre, performed with t he Sigma/GRANAT telescope. We determine the locations of the nine hard X-ray sources-six of them being observed for the first time in the sp ectral band-to an accuracy of about 2 arcmin, but find no source assoc iated with Sgr A. The hard X-ray luminosity of Sgr A* is a factor of. 4 x 10(7) less than that expected for a black hole of a million solar masses accreting gas at the maximum stable rate, challenging the idea that there is a black hole at the Galactic Centre.