SPECTRUM OF VY CANIS MAJORIS FROM 2.9 TO 14 MICRONS

被引:20
作者
GILLETT, FC
STEIN, WA
SOLOMON, PM
机构
关键词
D O I
10.1086/180553
中图分类号
P1 [天文学];
学科分类号
0704 ;
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页码:L173 / &
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共 13 条
[1]  
BECKLIN EE, 1970, PRIVATE COMMUNICATIO
[2]   OH EMISSION AND INFRARED STAR IN VY CANIS MAJORIS [J].
BOOTH, RS .
NATURE, 1969, 224 (5221) :783-&
[3]   STELLAR MOLECULAR ABUNDANCES .I. POLYATOMIC MOLECULES [J].
DOLAN, JF .
ASTROPHYSICAL JOURNAL, 1965, 142 (04) :1621-&
[4]   DISCOVERY OF AN INTENSE OH EMISSION SOURCE [J].
ELIASSON, B ;
BARTLETT, JF .
ASTROPHYSICAL JOURNAL, 1969, 155 (2P2) :L79-&
[5]  
HERBIG GH, 1969, 16 LIEG S
[6]  
HERZBERG G, 1950, MOLECULAR SPECTRA MO, V1
[7]   OBSERVATIONS OF INFRARED OBJECT, VY CANIS MAJORIS [J].
HYLAND, AR ;
BECKLIN, EE ;
NEUGEBAU.G ;
WALLERST.G .
ASTROPHYSICAL JOURNAL, 1969, 158 (2P1) :619-&
[8]   A POSSIBLE IDENTIFICATION OF INTERSTELLAR SILICATE ABSORPTION IN INFRARED SPECTRUM OF 119 TAURI [J].
KNACKE, RF ;
GAUSTAD, JE ;
GILLETT, FC ;
STEIN, WA .
ASTROPHYSICAL JOURNAL, 1969, 155 (3P2) :L189-&
[9]  
KNOWLES SH, 1969, SCIENCE, V163, P1057
[10]  
Neugebauer G., 1969, 2 MICRON SKY SURVEY