INFRARED OBSERVATIONS OF MASS-LOSS FROM MASSIVE STARS

被引：0
作者：
BARLOW, MJ
MOFFAT, AFJ
TAYLOR, MJ
BARLOW, MJ
LEITHERER, C
机构：
[1] UNIV MONTREAL, DEPT PHYS, MONTREAL H3C 3J7, QUEBEC, CANADA
[2] UNIV WISCONSIN, SPACE ASTRON LAB, MADISON, WI 53706 USA
[3] UNIV LONDON UNIV COLL, DEPT PHYS & ASTRON, LONDON WC1E 6BT, ENGLAND
[4] SPACE TELESCOPE SCI INST, BALTIMORE, MD 21218 USA
来源：
IAU SYMPOSIA | 1991年 / 143期
关键词：
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The future use of space-borne IR spectroscopy to determine the ionization structure and abundances in the outer winds of WR stars is described. A mass loss rate of 1.7 x 10(-5) M.yr-1 has been derived from 10-mu-m photometry of the WO2 star Sanduleak 5 (WR 142). The He/H number ratios in the winds of P Cyg and AG Car have been derived from a recombination line analysis of their 1-4-mu-m spectra and mass loss rates of 2.2 x 10(-5) M. yr-1 and 3.7 x 10(-5) M. yr-1 have been respectively derived for them.
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页码：281 / 287
页数：7
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