Hostname: page-component-78c5997874-8bhkd Total loading time: 0 Render date: 2024-11-14T08:23:00.677Z Has data issue: false hasContentIssue false
  • English
  • Français

Observed Mass Loss from Central Stars of Planetary Nebulae

Published online by Cambridge University Press:  07 August 2017

M. Perinotto
M. Perinotto*
Affiliation:
Dipartimento di Astronomia e Scienza dello Spazio, Universita' de Firenze

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

In the Introduction we recall the mass loss history of a progenitor of a planetary nebula (PN). Then we concentrate on the status of knowledge of fast winds in central stars of planetary nebulae (CSPN) : the detection and statistics, the observed edge velocities, relationships of the edge velocities with other stellar or nebular parameters. We then summarize the methods used to derive the mass loss rates associated to the fast winds, and review the determinations of the “observed” mass loss rates. The comparison with predictions from the radiation driven theory (RDT) is then discussed as well as possible lines for future improvements.

Type
II. Highlights on the Nuclei
Information
Symposium - International Astronomical Union , Volume 155: Planetary Nebulae , 1993 , pp. 57 - 64
Copyright
Copyright © Kluwer 1993 

References

Bianchi, L.: 1992, Astron. Astrophys. 253, 447.Google Scholar
Castor, J.I.: 1991, in Stellar Atmospheres: Beyond Classical Models , eds. Crivellari, L., Hubeny, I., Hummer, D. G., Kluwer Academic Publ., Dordrecht, p. 221.CrossRefGoogle Scholar
Cerruti-Sola, M., Perinotto, M.: 1985, Astrophys. J. 291, 237.CrossRefGoogle Scholar
Cerruti-Sola, M., Perinotto, M.: 1989, Astrophys. J. 345, 339.CrossRefGoogle Scholar
Feibelman, W.A., Bruhweiler, F.C.: 1989, Astrophys. J. 347, 901.CrossRefGoogle Scholar
Heap, S.: 1986, in New Insights in Astrophysics , ESA SP-263, p. 291.Google Scholar
Hutsemekers, D., Surdej, J.: 1989, Astron. Astrophys. 219, 237.Google Scholar
Iben, I. Jr., Renzini, A.: 1983, Ann. Rev. Astron. Astrophys. 21, 271.CrossRefGoogle Scholar
Kaler, J.B., Feibelman, W.A., Henrichs, H.F.: 1988, Astrophys. J. 324, 528.CrossRefGoogle Scholar
Kaler, J.B., Shaw, R.A., Feibelman, W.A., Lutz, J.H.: 1989, Astrophys. J. Suppl. 70, 213.CrossRefGoogle Scholar
Kudritzki, R.P., Pauldrach, A.W.A., Puls, J., Abbott, D.C.: 1989, Astron. Astrophys. 219, 205.Google Scholar
Kudritzki, R.P., Hummer, D.G., Pauldrach, A.W.A., Puls, J., Najarro, F., Imhoff, J.: 1992, Astron. Astrophys. 257, 655.Google Scholar
Lamers, H.J.G.L.M.: 1991, in Stellar Atmospheres: Beyond Classical Models , NATO ASI Ser. Conference, eds. Crivellari, L., Hubeny, I., Hummer, D.G., Kluwer Academic Publ., Dordrecht, p. 311.CrossRefGoogle Scholar
Meaburn, J., Walsh, J.R.: 1980, Mon. Not. R. astr. Soc. 191, 5p.Google Scholar
Patriarchi, P., Perinotto, M.: 1991, Astron. Astrophys. Suppl. 91, 325.Google Scholar
Pauldrach, A.W.A., Puls, J., Kudritzki, R.P., Mendez, R.H., Heap, S.R.: 1988, Astron. Astrophys. 207, 123.Google Scholar
Perinotto, M.: in IAU Symp. N. 131, Planetary Nebulae , ed. Torres-Peimbert, S., Reidel Publ., Dordrecht, p. 293.Google Scholar
Perinotto, M., Cerruti-Sola, M., Lamers, H.J.G.L.M.: 1989, Astrophys. J. 337, 382.CrossRefGoogle Scholar
Reimers, D.: 1975a, Mem. Soc. R. Sci. Liege, 6 Ser. , 8, 369.Google Scholar
Reimers, D.: 1975b, in Problems in Stellar Atmospheres and Envelopes , eds. Baschek, B., Kegel, W. H., Traving, G., Springer Publ., p. 229.CrossRefGoogle Scholar
Renzini, A.: 1981, in Physical Processes in Red Giants , eds. Iben, I. Jr., Renzini, A., Reidel Publ., Dordrecht, p. 165.CrossRefGoogle Scholar
Trams, N.R.: 1992, Thesis , Utrecht, SRON Laboratorium.Google Scholar
Werner, K., Koesterke, L.: 1992, in The Atmospheres of the Early-Type Stars , eds. Heber, U., Jeffery, C.S., Springer-Verlag, Berlin, p. 288.CrossRefGoogle Scholar