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Ring Nebulae Around of and WO Stars

Published online by Cambridge University Press:  03 August 2017

Tatiana A. Lozinskaya
Tatiana A. Lozinskaya*
Affiliation:
Sternberg State Astronomical Institute, Moscow, USSR

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To understand the origin of WR-rings it is of interest to consider nebulae associated with the precursors of WR stars and with stars at later stages of evolution. The former are represented by numerous Of stars and the latter by only four WO stars which, according to Barlow and Hummer (1982), are the most extreme WR stars near the end of their lives.

Type
Session VI. Enrichment
Information
Symposium - International Astronomical Union , Volume 143: Wolf–Rayet Stars and Interrelations with other Massive Stars in Galaxies , 1991 , pp. 365 - 370
Copyright
Copyright © Kluwer 1991 

References

Barlow, M.J., Hummer, D.G., 1982, in IAU Symp. No. 99. Wolf-Rayet Stars: Observations, Physics, Evolution. Eds. de Loore, C.W.H., Willis, A. J. (Dordrecht: Reidel), p. 387.Google Scholar
Cong, H.I.L., 1977, Ph.D. Thesis, Columbia University.Google Scholar
Dame, T.M., Ungerechts, H., Cohen, R.S., de Geus, E.J., Gremier, I.A., May, J., Murphy, D.C., Nyman, L.-R., Thaddeus, P., 1987, Astrophys. J. 322, 706.Google Scholar
Davies, R.D., Elliott, K.H., Meaburn, J., 1976, Mem. R. astr. Soc. 81, 89.Google Scholar
Dopita, M.A., Lozinskaya, T.A., McGregor, P.J., Rawlings, S.J., 1990, Astrophys. J. 351, 563.Google Scholar
Dopita, M.A., Lozinskaya, T.A., 1990, Astrophys. J. 359, 419.Google Scholar
Dyson, J.E., 1981, in: Investigating the Universe. Ed. Kahn, F. D. (Dordrecht: Reidel), p. 125.Google Scholar
Graham, J.R., 1985, Observatory 105, 7.Google Scholar
Isserstedt, J., 1984, Astron. Astrophys. 131, 347.Google Scholar
Kontizas, E., Morgan, D.H., 1988, Astron. Astrophys. 201, 208.Google Scholar
Loiseau, N., Klein, U., Greibe, A., Wielebinske, R., Haynes, R.F., 1987, Astron. Astrophys. 178, 62.Google Scholar
Lozinskaya, T.A., 1982, Astroph. Space Sci. 87, 313.CrossRefGoogle Scholar
Lozinskaya, T.A., 1986, Supernovae and stellar winds: the interaction with the ISM, Moscow, Nauka (AIP, New York, 1991).Google Scholar
Lozinskaya, T.A., Repin, S.V., 1990, Astron. Zh. (in press).Google Scholar
Lozinskaya, T.A., Sitnik, T.G., 1988, Pis'ma Astron. Zh. 14, 240 (= Sov. Astron. Letters 14, 100).Google Scholar
Mathewson, D.S., Ford, V.L., Visvanathan, N., 1988, Astrophys. J. 333, 617.Google Scholar
McGee, Newton, 1982, Proc. Astron. Soc. Austral. 4, 195.Google Scholar
Meaburn, J., 1980, Monthly Notices Roy. Astron. Soc. 192, 365.Google Scholar
Moffat, A.F.J., Breysacher, J., Seggewiss, W., 1985, Astrophys. J. 292, 511.Google Scholar
Pitault, A., 1981, Astron. Astrophys. 97, L5.Google Scholar
Torres, A.V., Conti, P.S., Massey, P., 1986, Astrophys. J. 300, 379.CrossRefGoogle Scholar
Turner, D.G., Forbes, D., 1982, Publ. Astron. Soc. Pacific 94, 789.Google Scholar
Wendker, H.J., 1984, Astron. Astrophys. Suppl. 59, 291.Google Scholar
Westerlund, B.E., 1964, Monthly Notices Roy. Astron. Soc. 127, 429.Google Scholar