Upper limits to X-ray emission from colliding stellar winds

Details Upper limits to X-ray emission from colliding stellar winds Upper limits to X-ray emission from colliding stellar winds

Jun 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978natur.273..645c&link_type=abstract

Nature, vol. 273, June 22, 1978, p. 645, 646. Research supported by the Radcliffe Trust and IBM Corp.

Astronomy and Astrophysics

Astronomy

35

Binary Stars, Stellar Winds, X Ray Astronomy, Electron Scattering, O Stars, Particle Collisions, Stellar Luminosity, Stellar Mass Ejection

Scientific paper

The X-ray emissions due to the collisions of stellar winds from binary stars are studied. The study considers the spectrum and intensity of radiation emitted by the shocked gas, as determined by the velocity and rate of mass loss in binary systems. X-ray emissions produced by colliding stellar winds during the birth processes of O stars are also discussed.

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