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