Hostname: page-component-5c6d5d7d68-wbk2r Total loading time: 0 Render date: 2024-09-01T21:19:16.789Z Has data issue: false hasContentIssue false
  • English
  • Français

Supergiant mass loss and the Cassiopeia A progenitor

Published online by Cambridge University Press:  14 August 2015

Susan A. Lamb
Susan A. Lamb*
Affiliation:
University of California, Los Angeles

Extract

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.

Observations of the chemical abundances in young supernova remnants may be used, in some circumstances, to place constraints on the evolution of the progenitor stars. For example, if a progenitor was massive (M > 10 M⊙), the presence of high 14N/1H ratios (that is, more than five time the solar value) in the supernova remnant can imply that substantial mass loss took place during the star's early evolution, that is, while it was an early-type supergiant.

Type
Session 6: Evolution with Mass Loss: Single Stars
Information
Symposium - International Astronomical Union , Volume 83: Mass Loss and Evolution of O-Type Stars , 1979 , pp. 357 - 365
Copyright
Copyright © Reidel 1979 

References

Arnett, W.D.: 1975, Astrophys. J., 195, 727.CrossRefGoogle Scholar
Barlow, M.J., and Cohen, M.: 1977, Astrophys. J., 213, 737.CrossRefGoogle Scholar
Charles, P.A., Culhane, J.L., Fabian, A.C.: 1977, Mon. Not. R. astr. Soc., 178, 307.CrossRefGoogle Scholar
Chevalier, R.A.: 1976, Astrophys. J., 208, 826.CrossRefGoogle Scholar
Chevalier, R.A. and Kirshner, R.P.: 1978, Astrophys. J., 219, 926.Google Scholar
Chiosi, C., Nasi, E., and Sreenivasan, S.R.: 1978, Astron. Astrophys., 63, 103.Google Scholar
Davidson, K.: 1973, Astrophys. J., 186, 223.Google Scholar
Davidson, K.: 1978, 'Emission-line Spectra of Condensations in the Crab Nebula (preprint) CrossRefGoogle Scholar
de Loore, C., De Grève, J.P., and Lamers, H.J.G.L.M.: 1977, Astron. Astrophys., 61, 251.Google Scholar
Endal, A.S.: 1975, Astrophys. J., 197, 405.Google Scholar
Hartwick, F.D.A.: 1967, Astrophys. J., 150, 953.CrossRefGoogle Scholar
Hutchings, J.B.: 1976, Astrophys. J., 203, 438.CrossRefGoogle Scholar
Kamper, K. and van den Bergh, S.: 1976, Astrophys. J. Suppl., 32, 351.CrossRefGoogle Scholar
Lamb, S.A.: 1978a, Astrophys. J., 220, 186.CrossRefGoogle Scholar
Lamb, S.A.: 1978b, ‘Evolution of a 50 M⊙ star’ (in preparation).Google Scholar
Lamb, S.A., Iben, I., and Howard, W.M.: 1976, Astrophys. J., 207, 209.CrossRefGoogle Scholar
Peimbert, M.: 1971, Astrophys. J., 170, 261.CrossRefGoogle Scholar
Peimbert, M. and van den Bergh, S.: 1971, Astrophys. J., 167, 223.CrossRefGoogle Scholar