A 21 MICRON EMISSION FEATURE IN 4 PROTO-PLANETARY NEBULAE

被引：188

作者：

KWOK, S

VOLK, KM

HRIVNAK, BJ

机构：

[1] NASA, AMES RES CTR, MOFFETT FIELD, CA 94035 USA

[2] VALPARAISO UNIV, DEPT PHYS, VALPARAISO, IN 46383 USA

来源：

ASTROPHYSICAL JOURNAL | 1989年 / 345卷 / 01期

关键词：

D O I：

10.1086/185550

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：L51 / L54

页数：4

共 17 条

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[7] GROUND-BASED INFRARED OBSERVATIONS OF VARIABLE IRAS SOURCES AS CANDIDATES FOR LATE ASYMPTOTIC GIANT BRANCH STARS [J].

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[8] GROUND-BASED OBSERVATIONS OF IRAS CANDIDATES FOR LATE ASYMPTOTIC GIANT BRANCH STARS [J].

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