ASCA X-RAY SPECTROSCOPY OF WR140 NEAR PERIASTRON

被引:0
作者
POLLOCK, AMT
CORCORAN, MF
STEVENS, IR
WILLIAMS, PM
VANDERHUCHT, KA
机构
[1] NASA,GODDARD SPACE FLIGHT CTR,HEASARC,GREENBELT,MD 20771
[2] UNIV BIRMINGHAM,SCH PHYS & SPACE RES,BIRMINGHAM B15 2TT,W MIDLANDS,ENGLAND
[3] ROYAL OBSERV,EDINBURGH EH9 3HJ,MIDLOTHIAN,SCOTLAND
[4] SRON,3584 CA UTRECHT,NETHERLANDS
来源
WOLF-RAYET STARS: BINARIES, COLLIDING WINDS, EVOLUTION | 1995年 / 163期
关键词
STARS; WOLF-RAYET; X-RAYS; CHEMICAL ABUNDANCES;
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Analysis of the X-ray spectrum of WR140 seven months after the 1993 periastron passage shows chemical abundances inconsistent with those used to model the earlier, more heavily absorbed, PV phase spectrum.
引用
收藏
页码:510 / 511
页数:2
相关论文
共 1 条
[1]  
WILLIAMS PM, 1990, MON NOT R ASTRON SOC, V243, P662