Colliding Winds in the WR+OB Binary θ Mus (WR 48)

Details Colliding Winds in the WR+OB Binary θ Mus (WR 48) Colliding Winds in the WR+OB Binary θ Mus (WR 48)

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aas...20111312h&link_type=abstract

American Astronomical Society, 201st AAS Meeting, #113.12; Bulletin of the American Astronomical Society, Vol. 34, p.1286

Astronomy and Astrophysics

Astronomy

Scientific paper

Spectra, providing full phase coverage, of the 19 d WC6+OB binary θ Mus (WR 48, HD 113904), have been obtained and show dramatic variations of the C iii λ 5696 emission line profile. We have modeled these line profile variations assuming the winds from the WR star and its close OB companion are colliding and forming a shock region from which extra emission originates.

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