Studies of blue supergiants in M31 and M33 with HIRES on the Keck I telescope

被引：0

作者：

McCarthy, JK ^{[1
]}

Venn, KA ^{[1
]}

Lennon, DJ ^{[1
]}

Kudritzki, RP ^{[1
]}

Puls, J ^{[1
]}

机构：

[1] CALTECH, Palomar Observ, Pasadena, CA 91125 USA

来源：

BOULDER-MUNICH II: PROPERTIES OF HOT, LUMINOUS STARS | 1997年 / 131卷

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：

Studies of the visually brightest stars, A- and B-type supergiants, in the Local Group galaxies M31 and M33 have been undertaken with HIRES on the 10-m Keck I telescope. Detailed chemical, element abundances are derived from these spectra (as reviewed at this conference by Venn); in this paper, we discuss the Keck observing program and the analysis of the H alpha line profile used to determine the stellar wind momentum. The current status of our tests of the Wind-momentum-Luminosity Relation in M31 and M33 is briefly summarized.

引用

页码：197 / 207

页数：11

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