Abstract
A conference on the theory of line formation (‘Second Harvard-Smithsonian Conference on Stellar Atmospheres’) was held in Cambridge, Mass., on 20–22 January 1965. The meeting was organized by the Smithsonian Astrophysical Observatory and the Harvard College Observatory. A fairly large number of papers were presented. There was a strong emphasis on non-LTE line formation problems for ‘few level’ atoms.
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(d) Thermodynamic problems of stellar atmospheres
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Vardya, M. S. 1965, Pressure Dissociation and Molecular Hydrogen. Mon. Not. R. astr. Soc., 129, 345. 10. Wyller, A., Morris, S. 1967 (submitted to Ann. Astrophys.).
(e) Extended envelopes
Brandt, J. C. 1966, Chemical composition of the photosphere and corona as influenced by the solar wind. Astrophys. J., 143, 265.
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f) General theory of line profiles and line formation
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Abhyankar, K. D. 1965, On the Schuster Problem for a Moving Atmosphere, III. Astrophys. J., 141, 1056.
Athay, R. G. 1964, Source-Function Equality in Multiplets. Astrophys. J., 140, 1579.
Athay, R. G. 1965, Theoretical Line Intensities. I. Strong Emission Lines. II. Excitation
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Athay, R. G. 1966, Theoretical Line Intensities. IV. Source Functions and Equivalent Widths. Astrophys. J., 144, 1159.
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Baschek, B., Holweger, H., Traving, G. 1966, Ein Algol-Programm für die Analyse von Sternspektren. Abh. Hamburger Sternwarte, 8, no. 1.
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Pagel, B. E. J. 1964, R. Obs. Bull., no. 87.
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III. Model Atmospheres and Theory of Spectra for Individual Stars or Groups of Stars, Methods
of Abundance Determination (a) ‘Normal’ stars (except Sun) and general literature on methods of abundance determination
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Wyller, A. 1966 (unpublished).
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© 1967 Springer Science+Business Media Dordrecht
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Böhm, K.H. (1967). Commission de la Theorie des Atmospheres Stellaires. In: Perek, L. (eds) Reports on Astronomy/Proceedings of the Thirteenth General Assembly Prague 1967. International Astronomical Union Transactions, vol 13B. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-3476-0_28
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