Observations of the variability in the MIR spectra of R CrB stars

被引：0
|
作者：
Heinrichsen, I [1 ]
Walker, HJ [1 ]
机构：
[1] Max Planck Inst Kernphys, D-69117 Heidelberg, Germany
来源：
FIRST ISO WORKSHOP ON ANALYTICAL SPECTROSCOPY: WITH SWS, LWS, PHT-S, AND CAM-CVF | 1997年 / 419卷
关键词：
circumstellar matter; stars; individual; variable; ABG and post-AGB; infrared;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
R CrB stars form a family of highly hydrogen deficient, late-type stars, which undergo deep minima in their visible light curve at irregular intervals. We present spectra of R CrB itself, observed at different times after minimum, and of RY Sgr, For this workshop paper we concentrate on the technical feasibility and problematics of the calibration of such variable measurements using PHT-S on ISOPHOT.
引用
收藏
页码：307 / 308
页数：2
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