OPTICAL-EMISSION BANDS IN THE SPECTRUM OF THE R-CRB STAR V854-CEN AT MINIMUM

被引：28

作者：

RAO, NK ^{[1
]}

LAMBERT, DL ^{[1
]}

机构：

[1] UNIV TEXAS,DEPT ASTRON,AUSTIN,TX 78712

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1993年 / 263卷 / 03期

关键词：

CIRCUMSTELLAR MATTER; STARS INDIVIDUAL V854-CEN; STARS VARIABLES OTHER; ISM MOLECULES;

D O I：

10.1093/mnras/263.1.L27

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Several unidentified broad emission features, previously seen only in the spectrum of the nebulosity in the Red Rectangle, have been observed in a spectrum of the R CrB star V854 Cen taken in a deep minimum. Similarities and differences between the bands from the two sources are noted. The presence of the bands associated with an R CrB star may suggest that their carrier does not contain hydrogen atoms. Extended red emission seen from the Red Rectangle and probably associated with hydrogenated carbon grains is not present in the spectrum of V854 Cen.

引用

页码：L27 / L31

页数：5

共 27 条

[1] THE INFRARED-EMISSION BANDS .1. CORRELATION STUDIES AND THE DEPENDENCE ON C/O RATIO [J].