THE DISCOVERY OF PULSED IRON LINE EMISSION FROM CENTAURUS X-3

被引:21
作者
DAY, CSR
NAGASE, F
ASAI, K
TAKESHIMA, T
机构
[1] INST SPACE & ASTRONAUT SCI,SAGAMIHARA,KANAGAWA 229,JAPAN
[2] INST PHYS & CHEM RES,WAKO,SAITAMA 35101,JAPAN
关键词
BINARIES; ECLIPSING; PULSARS; INDIVIDUAL (CENTAURUS X-3); STARS; X-RAYS;
D O I
10.1086/172625
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present the first discovery of pulsed iron line emission from an X-ray binary, namely Cen X-3. Compared with the continuum pulsations, the iron line pulsations are shallow (50% change in amplitude), smeared (the profile is a single-peaked sinusoid) and phase-shifted (by about half a cycle). We also discuss the constraints on the origin of the line imposed by this discovery and by other observations.
引用
收藏
页码:656 / 659
页数:4
相关论文
共 20 条
[1]  
Averintsev M. B., 1992, Soviet Astronomy, V36, P35
[2]  
DAY CSR, 1988, THESIS U CAMBRIDGE
[3]   X-RAY REFLECTION FROM COLD MATTER IN ACTIVE GALACTIC NUCLEI AND X-RAY BINARIES [J].
GEORGE, IM ;
FABIAN, AC .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1991, 249 (02) :352-367
[4]  
HAYASHIDA K, 1989, PUBL ASTRON SOC JPN, V41, P373
[5]   TENMA OBSERVATIONS OF BRIGHT BINARY-X-RAY SOURCES [J].
INOUE, H .
SPACE SCIENCE REVIEWS, 1985, 40 (1-2) :317-338
[6]   THE PULSE-PHASE DEPENDENCE OF THE SPECTRUM OF GX301-2 [J].
LEAHY, DA ;
MATSUOKA, M .
ASTROPHYSICAL JOURNAL, 1990, 355 (02) :627-634
[7]   TENMA OBSERVATIONS OF IRON LINE EMISSION FROM GX301-2 [J].
LEAHY, DA ;
MATSUOKA, M ;
KAWAI, N ;
MAKINO, F .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1989, 237 (02) :269-276
[8]  
MAKINO F, 1987, ASTROPHYS LETT COMM, V25, P223
[9]  
Makishima K., 1986, PHYSICS ACCRETION CO, P249
[10]  
NAGASE F, 1989, PUBL ASTRON SOC JPN, V41, P1