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The Influence of the Ratio of Total to Selective Extinction on the Determination of the Mass Loss Rate of Wolf Rayet Stars from Infrared Excess Measurements

Published online by Cambridge University Press:  14 August 2015

P.S. The ,
K.A. van der Hucht  and
M. Arens
P.S. The
Affiliation:
1Astronomical Institute, University of Amsterdam
K.A. van der Hucht
Affiliation:
2Space Research Laboratory, University of Utrecht
M. Arens
Affiliation:
1Astronomical Institute, University of Amsterdam

Abstract

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It is shown that the mass loss rate of the WN7 star HD 93162 decreases with larger values of the ratio of total to selective extinction R. for HD 93162 the mass loss rate will change one order of magnitude, only if ΔR ∼ 2. Mass loss rates are derived for nine other WR stars of which visual, red and near-infrared photometric observations were obtained.

Type
SESSION 3 — MASS-LOSS FROM WR STARS: OBSERVATIONS AND THEORY
Information
Symposium - International Astronomical Union , Volume 99: Wolf-Rayet Stars: Observations, Physics, Evolution , 1982 , pp. 197 - 201
Copyright
Copyright © Reidel 1982 

References

Barlow, M.J., Smith, L.J., and Willis, A.J.: 1981, Monthly Notices Roy. Astron. Soc. 196, 101.CrossRefGoogle Scholar
Dickel, H.R., Habing, H.J., and Isaacman, R.: 1980, Astrophys. J. (Letters) 238, L39.CrossRefGoogle Scholar
Forte, J.C.: 1978, Astron. J. 83, 1199.CrossRefGoogle Scholar
Hackwell, J.A., Gehrz, R.D., and Smith, J.R.: 1974, Astrophys. J. 192, 383.CrossRefGoogle Scholar
Herbst, W.: 1976, Astroph. J. 208, 923.CrossRefGoogle Scholar
Hidayat, B., Supelli, K., and van der Hucht, K.A.: 1981, these proceedings.Google Scholar
Hoffleit, D.: 1953, Ann. Harvard Coll. Obs. 119, No. 2.Google Scholar
van der Hucht, K.A., Conti, P.S., Lundström, I., and Stenholm, B.: 1981, Space Sci. Rev. 28, 227.CrossRefGoogle Scholar
Spitzer, L.: 1962, Physics of Fully Ionized Gases , 2nd ed., Interscience, New York, p. 148.Google Scholar
Thé, P.S., Bakker, R., Tjin A Djie, H.R.E.: 1980a, Astron. Astroph. 89, 209.Google Scholar
Thé, P.S., Bakker, R., Antalova, A.: 1980b, Astron. Astroph. Suppl. Ser. 41, 93.Google Scholar
Turner, D.G., Moffat, A.F.J.: 1980, Mon. Not. Roy. Astr. Soc. 192, 283.CrossRefGoogle Scholar
Willis, A.J.: 1981, in Chiosi, C. and Stalio, R. (eds), Effects of Mass Loss on Stellar Evolution , IAU Coll. 59, 27.CrossRefGoogle Scholar
Wright, A.E., Barlow, M.J.: 1975, Mon. Not. Roy. Astr. Soc. 170, 41.CrossRefGoogle Scholar