NEAR-INFRARED AND SUBMILLIMETER PHOTOMETRY OF CARBON STARS

被引：0
作者：
GROENEWEGEN, MAT
DEJONG, T
BAAS, F
机构：
[1] SRON,SPACE RES LAB,9700 AV GRONINGEN,NETHERLANDS
[2] JOINT ASTRON CTR,HILO,HI 96720
来源：
ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES | 1993年 / 101卷 / 03期
关键词：
STARS-CARBON; INFRARED-STARS;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We present J, H, K, L, M photometry for 25 carbon stars and 450, 600, 800 and 1100 mum fluxes for 12 carbon stars and the S-star W Aql. Carbon stars reside in a different part of the [12 - 25], [K-L] diagram than oxygen-rich stars. Our work confirms earlier observations and shows this relation to hold up to at least [K - L] almost-equal-to 8.
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页码：513 / 520
页数：8
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