The Nature of the 10 Kilosecond X-ray Flare in Sgr A*

Details The Nature of the 10 Kilosecond X-ray Flare in Sgr A* The Nature of the 10 Kilosecond X-ray Flare in Sgr A*

2001-09-06

arxiv.org/abs/astro-ph/0109081v2

Astronomy and Astrophysics

Astrophysics

Astronomy & Astrophysics Letters, in press, 4 pages, 3 figures, also available at http://www.mpifr-bonn.mpg.de/staff/hfalcke

Scientific paper

10.1051/0004-6361:20011346

The X-ray mission Chandra has observed a dramatic X-ray flare -- a brightening by a factor of 50 for only three hours -- from Sgr A*, the Galactic Center supermassive black hole. Sgr A* has never shown variability of this amplitude in the radio and we therefore argue that a jump of this order in the accretion rate does not seem the likely cause. Based on our model for jet-dominated emission in the quiescent state of Sgr A*, we suggest that the flare is a consequence of extra electron heating near the black hole. This can either lead to direct heating of thermal electrons to T_e~6*10^11 K and significantly increased synchrotron-self Compton emission, or result from non-thermal particle acceleration with increased synchrotron radiation and electron Lorentz factors up to gamma_e>10^5. While the former scenario is currently favored by the data, simultaneous VLBI, submm, mid-infrared and X-ray observations should ultimately be able to distinguish between the two cases.

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