X-ray velocity profiles round the orbit of WR140

Physics

Scientific paper

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Scientific paper

The orbit of the most brilliant eccentric WC7+O5 colliding-wind binary system WR140 up to the 2009 January periastron passage has given the opportunity to make direct measurements of the collisionless plasma at different phases. The clear differences are compared with the predictions of analytical and numerical models of the physics and dynamics and used to prepare the ground for future measurements of similar systems.

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