OBSERVATIONAL CONSTRAINTS ON DRIVING MECHANISMS FOR SPIRAL DENSITY WAVES

被引:219
作者
KORMENDY, J
NORMAN, CA
机构
[1] INST ASTRON,CAMBRIDGE CB3 0HA,ENGLAND
[2] RIJKSUNIV LEIDEN,HUYGENS LAB,NL-2300 RA LEIDEN,NETHERLANDS
关键词
D O I
10.1086/157414
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
引用
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页码:539 / &
相关论文
共 140 条
[1]   ATLAS OF PECULIAR GALAXIES [J].
ARP, H .
ASTROPHYSICAL JOURNAL, 1966, S 14 :1-&
[2]  
BARBON R, 1976, ASTRON ASTROPHYS, V49, P125
[3]  
BARDEEN J, 1978, COMMUNICATION
[4]  
BENVENUTI P, 1976, ASTRON ASTROPHYS, V53, P141
[5]  
BENVENUTI P, 1975, STARS GALAXIES OBSER, P393
[6]   DISCRETE SPIRAL MODES IN DISK GALAXIES - SOME NUMERICAL EXAMPLES BASED ON DENSITY WAVE THEORY [J].
BERTIN, G ;
LAU, YY ;
LIN, CC ;
MARK, JWK ;
SUGIYAMA, L .
PROCEEDINGS OF THE NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF AMERICA, 1977, 74 (11) :4726-4729
[7]  
BERTOLA F, 1973, ASTROPHYS LETT COMM, V13, P161
[8]  
BERTOLA F, 1966, MEM SOC ASTRON ITAL, V37, P433
[9]   ROTATION CURVES AND MASS DISTRIBUTIONS OF CLOSE PAIR OF SPIRAL GALAXIES NGC935 AND IC1801 [J].
BLACKMAN, CP .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1977, 178 (01) :15-26
[10]  
BOSMA A, 1977, ASTRON ASTROPHYS, V57, P373