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Galactic Wolf-Rayet Distribution and IMF

Published online by Cambridge University Press:  03 August 2017

Bambang Hidayat
Bambang Hidayat*
Affiliation:
Observatorium Bosscha, 1TB Lembang, West Java, Indonesia

Abstract

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Wolf-Rayet star to OB star number ratios in some selected regions in the Galaxy are presented. The variations of the number ratio as a function of location is found to be marginal.

Type
Session VIII. Inventory and Distribution
Information
Symposium - International Astronomical Union , Volume 143: Wolf–Rayet Stars and Interrelations with other Massive Stars in Galaxies , 1991 , pp. 587 - 590
Copyright
Copyright © Kluwer 1991 

References

Arnault, Ph., Kunth, D., Schild, H. 1989, Astron. Astrophys. 224, 73.Google Scholar
van den Bergh, S. 1986, Astrophys. Space Sci. 118, 435.CrossRefGoogle Scholar
Blitz, L., Spergel, D.N. 1989, Bull. American Astron. Soc. 21, 1189.Google Scholar
Bok, B. 1981, H.N. Russell Lecture, Publ. Steward Obs. No. 435.Google Scholar
Conti, P.S., Garmany, C.D., de Loore, C., Vanbeveren, D. 1983, Astrophys. J. 274, 302.CrossRefGoogle Scholar
Conti, P.S., Vacca, W.D. 1990, Astron. J. 100, 431.CrossRefGoogle Scholar
FitzGerald, M.P., Moffat, A.F.J. 1976, Astron. Astrophys. 50, 149.Google Scholar
Garmany, C.D., Conti, P.S., Chiosi, C. 1982, Astrophys. J. 263, 777.CrossRefGoogle Scholar
van der Hucht, K.A., Hidayat, B., Admiranto, A.G., Supelli, K.R., Doom, C. 1988, Astron. Astrophys. 199, 217.Google Scholar
Miller, G.E., Scalo, J.M. 1979, Astrophys. J. Suppl. 41, 533.CrossRefGoogle Scholar
Raharto, M. 1990, in: Proc. 5th Asian-Pacific Regional IAU Meeting, Sydney, Australia, in press.Google Scholar
Smith, L.F. 1968, Monthly Notices Roy. Astron. Soc. 141, 317.CrossRefGoogle Scholar