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On the Formation of Lithium Emission Lines in Nova Shells

Published online by Cambridge University Press:  25 May 2016

Marcos Diaz
Marcos Diaz*
Affiliation:
Instituto Astronômico e Geofísico - Universidade de São Paulo, 04301-904, São Paulo, SP, Brazil

Abstract

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The role of nova outbursts in the galactic lithium production is still controversial. Photoionization model calculations of nova shells are presented in this contribution, aiming to identify the optimal post-outburst phase for detecting lithium emission lines from nova ejecta which may confirm its lithium enhancement. Predictions for the Li I λ6708 Â flux are made as a function of the envelope geometry, its physical parameters and properties of the central ionizing source.

Type
6. Stellar Knowledge to and from Light Elements
Information
Symposium - International Astronomical Union , Volume 198: The Light Elements and their Evolution , 2000 , pp. 518 - 519
Copyright
Copyright © Astronomical Society of the Pacific 2000 

References

Diaz, M. 1998, in Science with Gemini, eds. Barbuy, , Lapaset, , Baptista, , & Fernandes, , (Santa Catarina:UFSC).Google Scholar
Diaz, M., Williams, R., Phillips, M., & Hamuy, M. 1995, MNRAS, 277, 959.CrossRefGoogle Scholar
Ferland, G. 1998, Korista, K., Vernet, D., Fergunson, J., Kingdon, J., & Verner, E. 1998, PASP, 110, 761.CrossRefGoogle Scholar
Gehrz, R., Truran, J., Williams, R., & Starrfield, S. 1998, PASP, 110, 3.CrossRefGoogle Scholar
Hernanz, M., Jose, J., Coc, A., & Isern, J. 1996, ApJ, 465, L27.CrossRefGoogle Scholar
Rauch, T. 1997, A&A, 320, 237.Google Scholar
Starrfield, S., Truran, J., Sparks, W., & Arnould, M. 1978, ApJ, 222, 600.CrossRefGoogle Scholar
Williams, R.E. 1992, ApJ, 376, 721.CrossRefGoogle Scholar