EXACT STUDY OF RIGIDLY AND RAPIDLY ROTATING STARS IN GENERAL RELATIVITY WITH APPLICATION TO CRAB PULSAR

被引：45

作者：

BONAZZOLA, S ^{[1
]}

SCHNEIDER, J ^{[1
]}

机构：

[1] OBSERV MEUDON, GRP ASTROPHYS RELATIVISTE, 92190 MEUDON, FRANCE

来源：

关键词：

D O I：

10.1086/152965

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：273 / 286

页数：14

共 28 条

[1]

ABRAMOWITZ M, 1964, HDB MATHEMATICAL FUN

[2] SOLIDIFICATION PRESSURE OF NUCLEAR AND NEUTRON STAR MATTER [J].

ANDERSON, PW ;

PALMER, RG .

NATURE-PHYSICAL SCIENCE, 1971, 231 (24) :145-&

[3] REEXAMINATION OF POST-NEWTONIAN MACLAURIN SPHEROIDS [J].

BARDEEN, JM .

[4]

BONAZZOLA S, 1973, AP J, V182, P334

[5]

BONAZZOLA S, 1971, CRAB NEBULA, P346

[6] ROTATING FLUID MASSES IN GENERAL RELATIVITY [J].

BOYER, RH .

PROCEEDINGS OF THE CAMBRIDGE PHILOSOPHICAL SOCIETY-MATHEMATICAL AND PHYSICAL SCIENCES, 1965, 61 :527-&

[7]

CANUTO V, 1972, PHYSICS DENSE MATTER

CHANDRAS.S .

CHANDRASEKHAR, S .

[10]

Chandrasekhar S., 1969, Ellipsoidal figures of equilibrium