Mining the IRAS database for proto-planetary nebulae

被引：0
|
作者：
Hrivnak, BJ [1 ]
Kwok, S [1 ]
Volk, K [1 ]
机构：
[1] Valparaiso Univ, Valparaiso, IN 46383 USA
来源：
ASTROPHYSICS WITH INFRARED SURVEYS: A PRELUDE TO SIRTF | 1999年 / 177卷
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D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The IRAS database has been used to identify proto-planetary nebulae candidates based upon their expected infrared excesses due to a detached circumstellar dust shell. This has permitted us to carry out a very successful multi-wavelength study (photometry, spectroscopy, imaging), which has contributed to a great advance in our understanding of these rare transitional objects.
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页码：369 / 372
页数：4
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