HOW BIG ARE SUPERMASSIVE BLACK-HOLES FORMED FROM THE COLLAPSE OF DENSE STAR-CLUSTERS

被引:12
作者
KOCHANEK, CS
SHAPIRO, SL
TEUKOLSKY, SA
机构
[1] CORNELL UNIV,CTR RADIOPHYS & SPACE RES,ITHACA,NY 14853
[2] CORNELL UNIV,DEPT PHYS & ASTRON,ITHACA,NY 14853
关键词
D O I
10.1086/165524
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
引用
收藏
页码:73 / 84
页数:12
相关论文
共 17 条
[1]   THEORY OF EXTRAGALACTIC RADIO-SOURCES [J].
BEGELMAN, MC ;
BLANDFORD, RD ;
REES, MJ .
REVIEWS OF MODERN PHYSICS, 1984, 56 (02) :255-351
[2]   STAR-CLUSTERS CONTAINING MASSIVE, CENTRAL BLACK-HOLES .4. GALACTIC TIDAL FIELDS [J].
DUNCAN, MJ ;
SHAPIRO, SL .
ASTROPHYSICAL JOURNAL, 1982, 253 (02) :921-938
[3]   MONTE-CARLO SIMULATIONS OF THE EVOLUTION OF GALACTIC NUCLEI CONTAINING MASSIVE, CENTRAL BLACK-HOLES [J].
DUNCAN, MJ ;
SHAPIRO, SL .
ASTROPHYSICAL JOURNAL, 1983, 268 (02) :565-581
[5]   RELATIVISTIC SPHERICALLY SYMMETRIC STAR CLUSTERS .I. STABILITY THEORY FOR RADIAL PERTURBATIONS [J].
IPSER, JR ;
THORNE, KS .
ASTROPHYSICAL JOURNAL, 1968, 154 (1P1) :251-+
[8]   LUMINOSITY EVOLUTION OF QUASARS AND ACTIVE GALAXIES - THEORETICAL-MODELS OF THE EVOLVING MASS SUPPLY RATE [J].
MCMILLAN, SLW ;
LIGHTMAN, AP ;
COHN, H .
ASTROPHYSICAL JOURNAL, 1981, 251 (02) :436-445
[9]  
Misner C. W., 2017, GRAVITATION
[10]  
QUINLAN GD, 1987, IN PRESS AP J