NEUTRON STAR MODELS BASED ON AN IMPROVED EQUATION OF STATE

[1] CAMERON AGW, 1969, ASTROPHYS LETT, V3, P3

[2] DYNAMICAL INSTABILITY OF GASEOUS MASSES APPROACHING SCHWARZSCHILD LIMIT IN GENERAL RELATIVITY [J]. ASTROPHYSICAL JOURNAL, 1964, 140 (02) : 417 - &

[3] Chandrasekhar S., 1935, MON NOT R ASTRON SOC, V95, P207

[4] CHIU HY, TO BE PUBLISHED

[5] CHIU HY, 1968, STELLAR PHYSICS, V1

[6] COCKE WJ, 1968, NATURE, V219, P1009, DOI 10.1038/2191009a0

[7] COCKE WJ, 1969, PULSATING STARS

[8] COCKE WJ, 1965, AM I HENRI POINCARE, V4, P238

[9] COHEN J, TO BE PUBLISHED

[10] EXACT FIELDS OF CHARGE AND MASS DISTRIBUTIONS IN GENERAL RELATIVITY [J]. NUOVO CIMENTO DELLA SOCIETA ITALIANA DI FISICA B-GENERAL PHYSICS RELATIVITY ASTRONOMY AND MATHEMATICAL PHYSICS AND METHODS, 1969, 60 (02): : 241 - &

[1] CAMERON AGW, 1969, ASTROPHYS LETT, V3, P3

[2] DYNAMICAL INSTABILITY OF GASEOUS MASSES APPROACHING SCHWARZSCHILD LIMIT IN GENERAL RELATIVITY [J]. ASTROPHYSICAL JOURNAL, 1964, 140 (02) : 417 - &

[3] Chandrasekhar S., 1935, MON NOT R ASTRON SOC, V95, P207

[4] CHIU HY, TO BE PUBLISHED

[5] CHIU HY, 1968, STELLAR PHYSICS, V1

[6] COCKE WJ, 1968, NATURE, V219, P1009, DOI 10.1038/2191009a0

[7] COCKE WJ, 1969, PULSATING STARS

[8] COCKE WJ, 1965, AM I HENRI POINCARE, V4, P238

[9] COHEN J, TO BE PUBLISHED

[10] EXACT FIELDS OF CHARGE AND MASS DISTRIBUTIONS IN GENERAL RELATIVITY [J]. NUOVO CIMENTO DELLA SOCIETA ITALIANA DI FISICA B-GENERAL PHYSICS RELATIVITY ASTRONOMY AND MATHEMATICAL PHYSICS AND METHODS, 1969, 60 (02): : 241 - &