Discrete sources as the origin of the Galactic X-ray ridge emission

Details Discrete sources as the origin of the Galactic X-ray ridge emission Discrete sources as the origin of the Galactic X-ray ridge emission

2009-04-29

arxiv.org/abs/0904.4649v1

Astronomy and Astrophysics

Astrophysics

Galaxy Astrophysics

16 pages, 3 figures. Draft version of the paper that will appear in Nature, Issue April 30, 2009

Scientific paper

10.1038/nature07946

An unresolved X-ray glow (at energies above a few kiloelectronvolts) was discovered about 25 years ago and found to be coincident with the Galactic disk -the Galactic ridge X-ray emission. This emission has a spectrum characteristic of a 1e8 K optically thin thermal plasma, with a prominent iron emission line at 6.7 keV. The gravitational well of the Galactic disk, however, is far too shallow to confine such a hot interstellar medium; instead, it would flow away at a velocity of a few thousand kilometres per second, exceeding the speed of sound in gas. To replenish the energy losses requires a source of 10^{43} erg/s, exceeding by orders of magnitude all plausible energy sources in the Milky Way. An alternative is that the hot plasma is bound to a multitude of faint sources, which is supported by the recently observed similarities in the X-ray and near-infrared surface brightness distributions (the latter traces the Galactic stellar distribution). Here we report that at energies of 6-7 keV, more than 80 per cent of the seemingly diffuse X-ray emission is resolved into discrete sources, probably accreting white dwarfs and coronally active stars.

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