X-ray emission from the giant molecular clouds in the Galactic Center region and the discovery of new X-ray sources

Details X-ray emission from the giant molecular clouds in the Galactic Center region and the discovery of new X-ray sources X-ray emission from the giant molecular clouds in the Galactic Center region and the discovery of new X-ray sources

2001-04-06

arxiv.org/abs/astro-ph/0104121v1

Astronomy and Astrophysics

Astrophysics

12 pages, 8 figures, accepted for publication in Astronomy & Astrophysics Main Journal

Scientific paper

10.1051/0004-6361:20010503

We report the results of X-ray (2-10 keV) observations of the giant molecular clouds SgrB, SgrC and SgrD in the Galactic Center region, together with the discovery of the point-like source SAXJ1748.2-2808. The data have been obtained with the MECS instrument on the BeppoSAX satellite. The core of SgrB2 has an X-ray luminosity of 6x10^34 erg/s and its spectrum is characterized by a strong Fe emission line at 6.5 keV with an equivalent width of 2 keV. Faint diffuse X-ray emission is detected from SgrC and from the SNR G1.05-0.15 (SgrD). A new, unresolved source with a strong Fe line has been discovered in the SgrD region. This source, SAXJ1748.2-2808, is probably associated with a SiO and OH maser source at the Galactic Center distance. If so, its luminosity is 10^34 erg/s. We propose that the X-ray emission from SAX J1748.2-2808 is produced either by protostars or by a giant molecular cloud core. Emission from sources similar to SAX J1748.2-2808 could have an impact on the expected contribution on the observed Fe line emission from the Galactic ridge.

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