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LTE Models

Published online by Cambridge University Press:  14 August 2015

Robert L. Kurucz
Robert L. Kurucz*
Affiliation:
Harvard-Smithsonian Center for Astrophysics 60 Garden St., Cambridge, MA 02138, USA

Abstract

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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.

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. 496–501.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. 87–97.Google Scholar
Kurucz, R.L. and Avrett, E.H. (1981) SAO Special Report No. 391. 139 pp.Google Scholar