An X-Ray Study of Two B+B Binaries: AH Cep and CW Cep
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/850/i=1/a=82/pdf
Reference50 articles.
1. A Steady, Radiative‐Shock Method for Computing X‐Ray Emission from Colliding Stellar Winds in Close, Massive‐Star Binaries
2. Exact, Algebraic Solutions of the Thin-Shell Two-Wind Interaction Problem
3. Radiation-driven winds in Of stars
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2. Modelling of the B-type binaries CW Cephei and U Ophiuchi;Astronomy & Astrophysics;2019-07-30
3. Physical properties and CNO abundances for high-mass stars in four main-sequence detached eclipsing binaries: V478 Cyg, AH Cep, V453 Cyg and V578 Mon;Monthly Notices of the Royal Astronomical Society;2018-09-14
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