EVIDENCE FOR AN 11.2 DAY PERIODICITY FROM CYGNUS X-2

被引：15

作者：

HOLT, SS

BOLDT, EA

SERLEMITSOS, PJ

KALUZIENSKI, LJ

机构：

[1] NASA GODDARD SPACE FLIGHT CTR,GREENBELT,MD 20771

[2] UNIV MARYLAND,COLLEGE PK,MD

来源：

ASTROPHYSICAL JOURNAL | 1976年 / 205卷 / 03期

关键词：

D O I：

10.1086/182109

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：L143 / L145

页数：3

共 7 条

[1]

CHEVALIER C, 1975, IAU2859 CIRC

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CRAMPTON, D .

ASTROPHYSICAL JOURNAL, 1975, 201 (02) :L65-L68

[3]

GIACCONI R, 1967, ASTROPHYS J, V148, pL129

[4] OPTICAL STUDIES OF UHURU SOURCES .11. PROBABLE PERIOD FOR SCORPIUS X-1 = V818 SCORPII [J].

GOTTLIEB, EW ;

WRIGHT, EL ;

LILLER, W .

ASTROPHYSICAL JOURNAL, 1975, 195 (01) :L33-L35

[5]

HOLT SS, IN PRESS

[6] PHOTOELECTRIC SCANNER SPECTROPHOTOMETRY OF CYG X-2 [J].

PEIMBERT, M ;

SPINRAD, H ;

TAYLOR, BJ ;

JOHNSON, HM .

ASTROPHYSICAL JOURNAL, 1968, 151 (2P2) :L93-&

[7] LONG-TERM OBSERVATIONS OF CYGNUS X-2 FROM OSO-7 [J].

ULMER, MP ;

SAMMULI, A ;

BAITY, WA ;

WHEATON, WA ;

PETERSON, LE .

ASTROPHYSICAL JOURNAL, 1974, 189 (02) :339-341

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