RADIATIVE TRANSFER EFFECTS ON THE COLORS OF RR LYRAE STARS

Автор(и)

  • C. G. Davis University of California, LOS Alamos National Lab., США

DOI:

https://doi.org/10.18524/1810-4215.1997.10.108172

Ключові слова:

Stars, RR Lyr-type, radiation transfer

Анотація

The methods of Davis and Cox (1980), are applied to a series of models described by Bono and Stellingwerf  (1994) to deter-mine the colors of RR Lyrae stars. Convection is ignored and the radiation flow is treated by a complete variable Eddington, multi-frequency dependent radiative transfer approximation.

Посилання

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Christy R.F.: 1966. ApJ, 145, 337

Cox A. N., Davis C.G.: 1975. ”Theoretical Mean Colors of Pulsating Cepheids” Memoire Societe, Royale de Liege. 6. Serie Tome VI.

Davis C.G.: 1971, JQSRT. 11, 647.

Davis C.G.: 1972, ApJ. 172, 419

Davis C.G.: 1974, ApJ, 187, 175

Davis C.G., Cox A.N.: 1980. In Current Problems in Stellar Pulsation Instabilities ed. D. Fischel, et. al. (NASA TM 80265). 293. (DC)

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Опубліковано

2017-08-01

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