An X-ray Binary Model for the Galactic Center Source IRS 13E

Details An X-ray Binary Model for the Galactic Center Source IRS 13E An X-ray Binary Model for the Galactic Center Source IRS 13E

2000-08-04

arxiv.org/abs/astro-ph/0008091v1

Astronomy and Astrophysics

Astrophysics

5 pages, 3 figures, accepted by A&A Letters

Scientific paper

We present several models for IRS 13E, an infrared, mm and X-ray source in the Galactic Center. Our favored interpretation is that of an early-type binary with strong colliding winds emission. This naturally explains the observed X-ray count rate and the strong infrared emission lines, and has a distinct advantage over competing hypotheses based upon a single star or black-hole system.

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