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Binary Wolf-Rayet Stars

Published online by Cambridge University Press:  14 August 2015

B. Hidayat  and
K. A. van der Hucht
B. Hidayat
Affiliation:
Observatorium Bosscha, ITB, Lembang, Indonesia
K. A. van der Hucht
Affiliation:
SRON Space Research Utrecht, The Netherlands

Abstract

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The distribution of the WR cluster members is interpreted in terms of their association with the galactic spiral-arm pattern. It is suggested that in a limited volume the number fraction of WR binaries is influenced more by magnetic field properties of the spiral arms, than by function of the galactocentric distance.

Type
Joint Discussions
Information
Highlights of Astronomy , Volume 8: Highlights of Astronomy. As presented at the XXth General Assembly of the IAU, 1988 , 1989 , pp. 153 - 154
Copyright
Copyright © Kluwer 1989

References

Bok, B., 1983, H.N. Russel Lecture, Publ.Steward Obs., No. 435.Google Scholar
Breysacher, J., 1980, Astron. Astrophys. Suppl. 43, 203.Google Scholar
Conti, P.S., Garmany, C.D., de Loore, C.W.H., and Vanbeveren, D., 1983, Ap. J. 234, 303.Google Scholar
Lundstrom, I. and Stenholm, B., 1984, Astron. Astrophys. Suppl. Ser. 58, 163.Google Scholar
Maeder, A., 1982, Astron. Astrophys. 105, 149.Google Scholar
Maeder, A., 1987, Astron. Astrophys. 173, 247.Google Scholar
Smith, L., 1988, Ap. J. 327, 128.Google Scholar
Van der Hucht, K.A., Hidayat, B., Admiranto, A.G., Supelli, K.R., and Doom, C., 1988, Astron. Astrophys. 199, 217.Google Scholar
Zinneker, H., 1982, in “Binary and Multiple Stars as Tracers of Stellar Evolution”, Kopal, Z. and Rahe, J. (eds.) Dordrecht, Reidel, P. 115.Google Scholar