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First Results of the Analysis of the Wolf-Rayet Star WR6

Published online by Cambridge University Press:  23 January 2015

Alex C. Gormaz-Matamala ,
Anthony Hervé ,
André-Nicolas Chené ,
Michel Curé  and
Ronald Mennickent
Alex C. Gormaz-Matamala
Affiliation:
Departamento de Astronomía, Universidad de Concepción, Casilla 160-C, Concepción, Chile email: [email protected]
Anthony Hervé
Affiliation:
CNRS & Université Montpellier II, Place Eugene Bataillon, F-34095 Montpellier, France
André-Nicolas Chené
Affiliation:
Gemini Observatory, Hawaii, USA.
Michel Curé
Affiliation:
Instituto de Física y Astronomía, Universidad de Valparaíso. Casilla 5030, Valparaíso, Chile
Ronald Mennickent
Affiliation:
Departamento de Astronomía, Universidad de Concepción, Casilla 160-C, Concepción, Chile email: [email protected]
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Abstract

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We present the first results of our analysis of the famous variable star, WR6 (HD50896). Using IUE ultraviolet data and an ESPaDOnS spectropolarimetric survey of this star, we plan to determine possible variation of the stellar and wind parameters during the different phases using the radiative transfer code CMFGEN. After the detection of parameter's modifications as a function of the phase, we will analyse deeper the origin of these variability (for example, CIRs?). In the present poster we show the first results of our analysis of the variability and the first step of the stellar parameter determination of the average spectrum of this star.

Keywords

AtmospheresMass LossWolf-Rayet
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Issue S307: New windows on massive stars: asteroseismology, interferometry, and spectropolarimetry , June 2014 , pp. 100 - 101
Copyright
Copyright © International Astronomical Union 2015 

References

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