A faint discrete source origin for the highly ionized iron emission from the Galactic Centre region

Author:

Wang Q. D.,Gotthelf E. V.,Lang C. C.

Publisher

Springer Science and Business Media LLC

Subject

Multidisciplinary

Reference26 articles.

1. Koyama, K. et al. ASCA view of our Galactic center: Remains of past activities in X-rays? Publ. Astron. Soc. J. 48, 249–255 (1996).

2. Sidoli, L. & Mereghetti, S. The X-ray diffuse emission from the Galactic center. Astron. Astrophys. 349, L49–L52 (1999).

3. Valinia, A. et al. On the origin of the iron K line in the spectrum of the Galactic X-ray background. Astrophys. J. 543, 733–739 (2000).

4. Tanaka, Y., Koyama, K., Maeda, Y. & Sonobe, T. Unusual properties of X-ray emission near the Galactic center. Publ. Astron. Soc. J. 52, L25–L30 (2000).

5. Wang, Q. D., Gotthelf, E. V., Lang, C. & Jagodzinski, F. UMass/Columbia Chandra X-ray survey of the Galactic center region. Astrophys. J. (submitted).

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