XMM-NewtonX-ray spectroscopy of the high-mass X-ray binary 4U 1700-37 at low flux
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361:20041288/pdf
Reference61 articles.
1. The origin of the runaway high-mass X-ray binary HD 153919/4U1700-37
2. Pile-up on X-ray CCD instruments
3. The mass of the neutron star in Vela X-1
4. The XSTAR Atomic Database
5. Hydrodynamic simulations of stellar wind disruption by a compact X-ray source
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1. Studying the variability of fluorescence emission and the presence of clumpy wind in HMXB GX 301−2 using XMM–Newton;Monthly Notices of the Royal Astronomical Society;2023-11-03
2. Spectroscopic modelling of two high-mass X-ray binaries, Cyg X–3 and 4U 1538–522;Monthly Notices of the Royal Astronomical Society;2021-08-02
3. High resolution X-ray spectroscopy of Supergiant HMXB 4U1700−37 during the compact object eclipse.;Monthly Notices of the Royal Astronomical Society;2020-12-26
4. High-resolution X-ray spectroscopy of the stellar wind in Vela X-1 during a flare;Astronomy & Astrophysics;2020-09
5. Possible detection of a new cyclotron feature in 4U 1700–37;Monthly Notices of the Royal Astronomical Society;2020-03-07
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