ELEMENTAL ABUNDANCE ANALYSES WITH DAO SPECTROGRAMS .11. THE EARLY B-STARS GAMMA-PEGASI AND IOTA-HERCULIS

被引：28

作者：

PINTADO, OI ^{[1
]}

ADELMAN, SJ ^{[1
]}

机构：

[1] THE CITADEL,DEPT PHYS,CHARLESTON,SC 29409

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1993年 / 264卷 / 01期

关键词：

STARS; ABUNDANCES; EARLY-TYPE; INDIVIDUAL; GAMMA PEG; IOTA HER;

D O I：

10.1093/mnras/264.1.63

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

This paper presents LTE analyses of two sharp-lined early B stars, gamma Pegasi and l Herculis, based on co-added IIaO and Reticon 2.4 A mm-1 spectrograms of the photographic region. Most of the derived abundances are close to solar. Both stars have definite microturbulences which probably are related to the instability of their photospheres.

引用

页码：63 / 70

页数：8