SK-71-DEGREES 34 - A NEW WOLF-RAYET STAR IN THE LARGE MAGELLANIC CLOUD

被引:23
作者
CONTI, PS [1 ]
GARMANY, CD [1 ]
机构
[1] UNIV COLORADO,NBS,JOINT INST LAB ASTROPHYS,BOULDER,CO 80309
关键词
D O I
10.1086/131185
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
引用
收藏
页码:411 / 412
页数:2
相关论文
共 13 条
[1]  
Bohannan B., 1974, Astronomy and Astrophysics Supplement Series, V18, P47
[2]  
Breysacher J., 1981, Astronomy & Astrophysics Supplement Series, V43, P203
[3]   SPECTROSCOPIC STUDIES OF O-TYPE STARS .1. CLASSIFICATION AND ABSOLUTE MAGNITUDES [J].
CONTI, PS ;
ALSCHULE.WR .
ASTROPHYSICAL JOURNAL, 1971, 170 (02) :325-&
[4]   THE SPECTRA OF WOLF-RAYET STARS .1. OPTICAL-LINE STRENGTHS AND THE HYDROGEN-TO-HELIUM RATIOS IN WN TYPE STARS [J].
CONTI, PS ;
LEEP, EM ;
PERRY, DN .
ASTROPHYSICAL JOURNAL, 1983, 268 (01) :228-245
[5]  
CONTI PS, 1982, IAU S, V99, P551
[6]   DISTANCE TO THE LARGE MAGELLANIC CLOUD FROM OB STARS [J].
CRAMPTON, D .
ASTROPHYSICAL JOURNAL, 1979, 230 (03) :717-723
[7]  
Henize K. G., 1956, AP J S, V2, P315
[8]  
Isserstedt J., 1979, Astronomy and Astrophysics Supplement Series, V38, P239
[9]   WOLF-RAYET STARS IN THE LMC - HOW FAINT ARE THE FAINTEST [J].
MASSEY, P ;
CONTI, PS .
ASTROPHYSICAL JOURNAL, 1983, 264 (01) :126-133
[10]  
SANDULEAK N, 1969, CERRO TOLOLO INTERAM, V89