ANALYTIC RELATIVISTIC MODEL FOR A SUPERDENSE STAR

[1] ADAMS RC, 1973, ASTROPHYS J, V198, P507

[2] ADLER R, 1974, J MATH PHYS, V15, P277

[3] MICROSCOPIC INTERPRETATION OF NEUTRON STAR STRUCTURE [J]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 1977, 33 (04) : 415 - 436

[4] BALDWIN JE, 1971, IAU S, V46, P226

[5] BAYM G, 1979, ANN REV ASTRON ASTRO, V17, P430

[6] BORNER G, 1973, SPRINGER TRACT MODER, V69

[7] OBESE NEUTRON STARS [J]. NATURE, 1976, 259 (5542) : 377 - 378

[8] CANUTO V, 1975, ANNU REV ASTRON ASTR, V13, P355

[9] MUST ULTRABARIC MATTER BE SUPERLUMINAL [J]. PHYSICAL REVIEW D, 1979, 20 (08): : 1823 - 1831

[10] DYNAMICAL INSTABILITY OF GASEOUS MASSES APPROACHING SCHWARZSCHILD LIMIT IN GENERAL RELATIVITY [J]. PHYSICAL REVIEW LETTERS, 1964, 12 (04) : 114 - &

[1] ADAMS RC, 1973, ASTROPHYS J, V198, P507

[2] ADLER R, 1974, J MATH PHYS, V15, P277

[3] MICROSCOPIC INTERPRETATION OF NEUTRON STAR STRUCTURE [J]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 1977, 33 (04) : 415 - 436

[4] BALDWIN JE, 1971, IAU S, V46, P226

[5] BAYM G, 1979, ANN REV ASTRON ASTRO, V17, P430

[6] BORNER G, 1973, SPRINGER TRACT MODER, V69

[7] OBESE NEUTRON STARS [J]. NATURE, 1976, 259 (5542) : 377 - 378

[8] CANUTO V, 1975, ANNU REV ASTRON ASTR, V13, P355

[9] MUST ULTRABARIC MATTER BE SUPERLUMINAL [J]. PHYSICAL REVIEW D, 1979, 20 (08): : 1823 - 1831

[10] DYNAMICAL INSTABILITY OF GASEOUS MASSES APPROACHING SCHWARZSCHILD LIMIT IN GENERAL RELATIVITY [J]. PHYSICAL REVIEW LETTERS, 1964, 12 (04) : 114 - &