Article contents
X-Ray Spectroscopy of the High-Mass X-Ray Binary 4U 1700-37
Published online by Cambridge University Press: 22 February 2018
Extract
We present the first results of a monitoring campaign of the high-mass X-ray binary system 4U 1700-37/HD 153919, carried out with XMM-Newton.
We have observed the high-mass X-ray binary (HMXB) 4U 1700-37 with XMM-Newton at four orbital phases in February 2001. 4U 1700-37 is powered by the dense stellar wind of the O supergiant HD 153919. Numerous X-ray flares are observed with a typical duration, of the order of half an hour. We focus on three intervals in which the data are not affected by pile up: the eclipse, the eclipse egress and a low-flux part around orbital phase ϕ ~ 0.28.
- Type
- The Contributed Papers
- Information
- Copyright
- Copyright © Instituto de astronomia/revista mexicana de astronomίa y astrofίsica 2004
References
- 1
- Cited by