Abstract
THE centre of our Galaxy is known to contain a large condensation of mass1, and it has been suggested that a massive black hole (of several million solar masses) is located there. Massive black holes have been proposed to explain active galactic nuclei, and if the Galactic Centre is a less-powerful version of such sources it should radiate X-rays and γ-rays1. But although earlier observations2–6 have shown that the region does emit X-rays and y-rays, the true centre, corresponding to the object Sagittarius A*, does not emit strongly at least 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 results of a deep imaging survey of the Galactic Centre, performed with the Sigma/GRANAT tele-scope. We determine the locations of the nine hard X-ray sources— six of them being observed for the first time in the spectral band— to an accuracy of about 2 arcmin, but find no source associated with Sgr A*. The hard X-ray luminosity of Sgr A* is a factor of 4 × 107 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.
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Goldwurm, A., Cordier, B., Paul, J. et al. Possible evidence against a massive black hole at the Galactic Centre. Nature 371, 589–591 (1994). https://doi.org/10.1038/371589a0
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DOI: https://doi.org/10.1038/371589a0
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