Volume 388, Number 1, June II 2002
|Page(s)||L20 - L23|
|Published online||28 May 2002|
Letter to the Editor
The dominant X-ray wind in massive star binaries
Department of Physics & Astronomy, The University of Leeds, Woodhouse Lane, Leeds, LS2 9JT, UK
2 Department of Physics & Astronomy, The University of Birmingham, Edgbaston, Birmingham, B15 2TT, UK
Corresponding author: J. M. Pittard, firstname.lastname@example.org
Accepted: 12 April 2002
We investigate which shocked wind is responsible for the majority of the X-ray emission in colliding wind binaries, an issue where there is some confusion in the literature, and which we show is more complicated than has been assumed. We find that where both winds rapidly cool (typically close binaries), the ratio of the wind speeds is often more important than the momentum ratio, because it controls the energy flux ratio, and the faster wind is generally the dominant emitter. When both winds are largely adiabatic (typically long-period binaries), the slower and denser wind will cool faster and the stronger wind generally dominates the X-ray luminosity.
Key words: stars: binaries: general / stars: early-type / stars: Wolf-Rayet / X-rays: stars
© ESO, 2002
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.