Properties of star 2, one of the SN 1987A companions, derived from Hubble space telescope faint object spectrograph observations

被引:35
|
作者
Scuderi, S
Panagia, N
Gilmozzi, R
Challis, PM
Kirshner, RP
机构
[1] ESA, DEPT SPACE SCI, DIV ASTROPHYS, FRASCATI, ITALY
[2] EUROPEAN SO OBSERV, D-8046 GARCHING, GERMANY
[3] HARVARD UNIV, CTR ASTROPHYS, CAMBRIDGE, MA 02138 USA
来源
ASTROPHYSICAL JOURNAL | 1996年 / 465卷 / 02期
关键词
binaries; visual; dust; extinction; stars; early-type; evolution; fundamental parameters; supernovae; individual; (SN; 1987A);
D O I
10.1086/177480
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present and discuss the Hubble Space Telescope Faint Object Spectrograph observations of Star 2, one of the two companions of SN 1987A, in the range 1200-8000 Angstrom. Our analysis, based on a comparison of the observed spectrum with spectra of O and B type stars and with model atmospheres, confirms that Star 2 is a B2III star. The extinction toward Star 2 is mostly of LMC origin and amounts to an E(B-V) = 0.19 +/- 0.02. The detailed extinction curve has a 2200 Angstrom bump less pronounced than the average LMC extinction law. Star 2 has an effective temperature of T-eff = 22,000 +/- 2000 K and a luminosity of log L/L. = 4.38 +/- 0.11. Also, Star 2 appears to rotate with an equatorial velocity of v sin i = 250 +/- 50 km s(-1) and is presently undergoing mass loss at a range of log M similar or equal to 7.0 +/- 0.5 M. yr(-1) Judging from its position in the H-R diagram and its present parameters, Star 2 had an original mass of about 13 M. and was born less than 13 Myr ago, which makes Star 2 coeval to the SN 1987A progenitor Sk 69 degrees 202.
引用
收藏
页码:956 / 964
页数:9
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