PRELIMINARY MODEL FOR X-RAY BINARY AM HERCULIS

被引：60

作者：

COWLEY, AP

CRAMPTON, D

机构：

[1] DOMINION ASTROPHYS OBSERV,VICTORIA V8X 3X3,BRITISH COLUMBI,CANADA

[2] UNIV MICHIGAN,DEPT ASTRON,ANN ARBOR,MI 48109

来源：

ASTROPHYSICAL JOURNAL | 1977年 / 212卷 / 03期

关键词：

D O I：

10.1086/182389

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：L121 / L124

页数：4

共 11 条

[1] NATURE OF AM-HERCULIS [J].

BERG, RA ;

DUTHIE, JG .

ASTROPHYSICAL JOURNAL, 1977, 211 (03) :859-865

[2] SPECTROSCOPIC SURVEY OF SOME HIGH LATITUDE BLUE VARIABLES [J].

BOND, HE ;

TIFFT, WG .

PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 1974, 86 (514) :981-984

[3]

COWLEY A, 1976, IAU2984 CIRC

[4]

HEARN D, 1976, COMMUNICATION

[5] DETECTION OF SOFT-X-RAY EMISSION FROM AN UNIDENTIFIED SOURCE AT HIGH GALACTIC LATITUDE [J].

HEARN, DR ;

RICHARDSON, JA ;

CLARK, GW .

ASTROPHYSICAL JOURNAL, 1976, 210 (01) :L23-L26

[6] BINARY STARS AMONG CATACLYSMIC VARIABLES .5. PHOTOELECTRIC + SPECTROSCOPIC OBSERVATIONS OF ULTRA-SHORT-PERIOD BINARY NOVA WZ SAGITTAE [J].

KRZEMINSKI, W ;

KRAFT, RP .

ASTROPHYSICAL JOURNAL, 1964, 140 (03) :921-&

[7]

MEINUNGER L, 1960, 524 VER STERN MITT

[8]

SMAK J, IN PRESS

[9] AM HERCULIS - UNIQUE X-RAY BINARY AS REVEALED THROUGH OPTICAL LIGHT-CURVE [J].

SZKODY, P ;

BROWNLEE, DE .

ASTROPHYSICAL JOURNAL, 1977, 212 (03) :L113-L116

[10]

TAPIA S, 1976, IAU2987 CIRC

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