HD 190918: Arbiter between models for Wolf-Rayet stars

Details HD 190918: Arbiter between models for Wolf-Rayet stars HD 190918: Arbiter between models for Wolf-Rayet stars

Mar 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ssrv...66..281u&link_type=abstract

Space Science Reviews, Volume 66, Issue 1-4, pp. 281-284

Physics

Scientific paper

New orbital elements for the 112.4 day WN4.5+O9.5Ia spectroscopic binary HD 190918 are presented. Solutions consistent with the O star being a main sequence star or a supergiant are obtained wheni=25° or 20°, respectively. We predict the X-ray flux to be expected from this system and note how an observation of the X-ray flux from HD 190918 would help one to choose the most probable value of the inclination.

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