APSIDAL-MOTION CONSTANTS FOR POLYTROPIC MODELS

[1] Chandrasekhar S., 1933, MON NOT R ASTRON SOC, V93, P390

[2] Chandrasekhar S., 1933, MON NOT R ASTRON SOC, V93, P539, DOI [10.1093/mnras/93.8.539a, DOI 10.1093/MNRAS/93.8.539A]

[3] CHANDRASEKHAR S, 1942, AP J, V95, P570

[4] A PROCESS FOR THE STEP-BY-STEP INTEGRATION OF DIFFERENTIAL EQUATIONS IN AN AUTOMATIC DIGITAL COMPUTING MACHINE [J]. PROCEEDINGS OF THE CAMBRIDGE PHILOSOPHICAL SOCIETY, 1951, 47 (01): : 96 - 108

[5] KELLER G, 1947, AP J, V108, P347

[6] KOPAL, 1946, INTRO STUDY ECLIPSIN, pCH6

[7] SOME REMARKS ON THE INTERPRETATION OF APSIDAL-MOTION CONSTANTS IN CLOSE BINARY SYSTEMS [J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1953, 113 (06) : 769 - 775

[8] THE APSIDAL MOTION AND RADIUS OF GYRATION OF THE PROTON-PROTON SOLAR MODEL [J]. ASTROPHYSICAL JOURNAL, 1953, 118 (01) : 147 - 150

[9] THE APSIDAL MOTION OF GIANT BINARY STARS [J]. ASTROPHYSICAL JOURNAL, 1950, 112 (03) : 434 - 444

[10] The apsidal motion in binary stars built on a point-source convenctive-core model with varying guillotine factor [J]. ASTROPHYSICAL JOURNAL, 1941, 94 (02) : 253 - 258

[1] Chandrasekhar S., 1933, MON NOT R ASTRON SOC, V93, P390

[2] Chandrasekhar S., 1933, MON NOT R ASTRON SOC, V93, P539, DOI [10.1093/mnras/93.8.539a, DOI 10.1093/MNRAS/93.8.539A]

[3] CHANDRASEKHAR S, 1942, AP J, V95, P570

[4] A PROCESS FOR THE STEP-BY-STEP INTEGRATION OF DIFFERENTIAL EQUATIONS IN AN AUTOMATIC DIGITAL COMPUTING MACHINE [J]. PROCEEDINGS OF THE CAMBRIDGE PHILOSOPHICAL SOCIETY, 1951, 47 (01): : 96 - 108

[5] KELLER G, 1947, AP J, V108, P347

[6] KOPAL, 1946, INTRO STUDY ECLIPSIN, pCH6

[7] SOME REMARKS ON THE INTERPRETATION OF APSIDAL-MOTION CONSTANTS IN CLOSE BINARY SYSTEMS [J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1953, 113 (06) : 769 - 775

[8] THE APSIDAL MOTION AND RADIUS OF GYRATION OF THE PROTON-PROTON SOLAR MODEL [J]. ASTROPHYSICAL JOURNAL, 1953, 118 (01) : 147 - 150

[9] THE APSIDAL MOTION OF GIANT BINARY STARS [J]. ASTROPHYSICAL JOURNAL, 1950, 112 (03) : 434 - 444

[10] The apsidal motion in binary stars built on a point-source convenctive-core model with varying guillotine factor [J]. ASTROPHYSICAL JOURNAL, 1941, 94 (02) : 253 - 258