On the carbon-star status of five stars in a new carbon star catalog

被引:16
作者
Chen, PS [1 ]
Gao, YF
机构
[1] Chinese Acad Sci, Natl Astron Observ, Yunan Observ, Kunming 650011, Peoples R China
[2] Chinese Acad Sci, Natl Astron Observ, Lab Opt Astron, Kunming 650011, Peoples R China
来源
CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS | 2002年 / 2卷 / 02期
关键词
stars : AGB; stars : carbon; infrared : stars;
D O I
10.1088/1009-9271/2/2/169
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We find that five sources listed in the new carbon star catalog are not really carbon-rich objects but oxygen-rich stars, because they all have the prominent 10mum silicate features in absorption and the 1612 MHz OH maser emission or/and the SiO molecular features. These objects were considered as carbon stars in the catalog based only on their locations in the infrared two-color diagram. Therefore to use the infrared two-color diagram to distinguish carbon-rich stars from oxygen-rich stars must be done with caution, because, in general, it has only a statistical meaning.
引用
收藏
页码:169 / 173
页数:5
相关论文
共 35 条
[1]  
ALKSNIS A, 2001, BALT ASTRON, V10, P1, DOI [10.1515/astro-2001-1-202, DOI 10.1515/ASTRO-2001-1-202]
[2]  
Barnbaum C, 1996, ASTRON ASTROPHYS, V310, P259
[3]   NEW SPECTRA OF CARBON STARS FROM THE IRAS LOW-RESOLUTION SPECTROMETER [J].
CHAN, SJ .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1994, 268 (01) :113-118
[4]  
Chen Peisheng, 1995, Acta Astronomica Sinica, V36, P394
[5]   Properties of OH/IR stars with IRAS LRS spectra [J].
Chen, PS ;
Szczerba, R ;
Kwok, S ;
Volk, K .
ASTRONOMY & ASTROPHYSICS, 2001, 368 (03) :1006-1020
[6]   CIRCUMSTELLAR PROPERTIES OF S-STARS .1. DUST FEATURES [J].
CHEN, PS ;
KWOK, S .
ASTROPHYSICAL JOURNAL, 1993, 416 (02) :769-786
[7]  
CHEN PS, 2001, UNPUB AJ
[8]  
CHEN PS, 1999, ACTA ASTRON SINICA, V40, P33
[9]   NEW OH IR STARS FROM COLOR-SELECTED IRAS SOURCES .3. A COMPLETE SURVEY [J].
CHENGALUR, JN ;
LEWIS, BM ;
EDER, J ;
TERZIAN, Y .
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 1993, 89 (01) :189-210
[10]  
DAVID P, 1993, ASTRON ASTROPHYS, V277, P453