Hostname: page-component-7bb8b95d7b-2h6rp Total loading time: 0 Render date: 2024-09-21T14:46:45.992Z Has data issue: false hasContentIssue false

LTE Models

Published online by Cambridge University Press:  14 August 2015

Robert L. Kurucz*
Affiliation:
Harvard-Smithsonian Center for Astrophysics60 Garden St., Cambridge, MA 02138, USA

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.

I can compute arbitrary-abundance models and spectra at high resolution using millions of atomic and diatomic molecular lines. Examples are given for Sakurai’s object and for a λBoo star. I am continuing to improve the input line data.

Type
II. Joint Discussions
Copyright
Copyright © Kluwer 1998

References

Allard, N.F., Kurucz, R.L., Gerbaldi, M., and Faraggiana, R. (1997) in preparation.Google Scholar
Castelli, F. and Kurucz, R.L. (1993) in Peculiar versus Normal Phenomena in A-type and Related Stars (eds. Dworetsky, M.M., Castelli, F., and Faraggiana, R.), A.S.P. Conference Series 44, pp. 496501.Google Scholar
Gautschy, A., Duerbeck, H.W., van Genderen, A.M., and Benetti, S. (1997) General Assembly abstract book p. 41.Google Scholar
Kerber, F., Gratl, H., Kimeswenger,S., and Weinberger, R. (1997) General Assembly abstract book p. 41.Google Scholar
Kurucz, R.L. (1993) in Peculiar versus Normal Phenomena in A-type and Related Stars (eds. Dworetsky, M.M., Castelli, F., and Faraggiana, R.), A.S.P. Conference Series 44, pp. 8797.Google Scholar
Kurucz, R.L. and Avrett, E.H. (1981) SAO Special Report No. 391. 139 pp.Google Scholar