MODELS FOR CARBON-RICH STARS WITH HELIUM ENVELOPES

[1] ALLER L, 1968, NEBULAE INTERSTELLAR

[2] CARBON-BURNING NUCLEOSYNTHESIS AT CONSTANT TEMPERATURE [J]. ASTROPHYSICAL JOURNAL, 1969, 157 (1P1) : 339 - &

[3] ENERGY LOSSES DUE TO NEUTRINO PROCESSES [J]. ASTROPHYSICAL JOURNAL, 1967, 150 (3P1) : 979 - +

[4] MODELS FOR CARBON-RICH STARS [J]. ASTROPHYSICAL JOURNAL, 1969, 155 (1P1) : 203 - &

[5] MODELS FOR INITIALLY HOMOGENEOUS CARBON-RICH STARS [J]. ASTROPHYSICAL JOURNAL, 1973, 181 (02) : 393 - 407

[6] Clayton D. D., 1968, PRINCIPLES STELLAR E

[7] Coetzee Greig, 2003, PRESS

[8] EQUILIBRIUM MODELS FOR STARS WHICH DERIVE ENERGY FROM HELIUM-BURNING .2. HELIUM STARS WITH HYDROGEN-RICH ENVELOPES [J]. ASTROPHYSICAL JOURNAL, 1961, 133 (03) : 764 - 780

[9] CRITICAL-LUMINOSITY IN STELLAR INTERIORS AND STELLAR SURFACE BOUNDARY-CONDITIONS [J]. ASTROPHYSICAL JOURNAL, 1973, 181 (02) : 429 - 438

[10] OSTERBROCK DE, 1970, Q J ROY ASTRON SOC, V11, P199

[1] ALLER L, 1968, NEBULAE INTERSTELLAR

[2] CARBON-BURNING NUCLEOSYNTHESIS AT CONSTANT TEMPERATURE [J]. ASTROPHYSICAL JOURNAL, 1969, 157 (1P1) : 339 - &

[3] ENERGY LOSSES DUE TO NEUTRINO PROCESSES [J]. ASTROPHYSICAL JOURNAL, 1967, 150 (3P1) : 979 - +

[4] MODELS FOR CARBON-RICH STARS [J]. ASTROPHYSICAL JOURNAL, 1969, 155 (1P1) : 203 - &

[5] MODELS FOR INITIALLY HOMOGENEOUS CARBON-RICH STARS [J]. ASTROPHYSICAL JOURNAL, 1973, 181 (02) : 393 - 407

[6] Clayton D. D., 1968, PRINCIPLES STELLAR E

[7] Coetzee Greig, 2003, PRESS

[8] EQUILIBRIUM MODELS FOR STARS WHICH DERIVE ENERGY FROM HELIUM-BURNING .2. HELIUM STARS WITH HYDROGEN-RICH ENVELOPES [J]. ASTROPHYSICAL JOURNAL, 1961, 133 (03) : 764 - 780

[9] CRITICAL-LUMINOSITY IN STELLAR INTERIORS AND STELLAR SURFACE BOUNDARY-CONDITIONS [J]. ASTROPHYSICAL JOURNAL, 1973, 181 (02) : 429 - 438

[10] OSTERBROCK DE, 1970, Q J ROY ASTRON SOC, V11, P199