EMISSION-LINE WIDTHS IN SPECTRUM OF POSSIBLE PROTO-PLANETARY NEBULA HM SAGITTAE

被引:40
作者
WALLERSTEIN, G
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10.1086/130274
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P1 [天文学];
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0704 ;
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页码:36 / 38
页数:3
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共 9 条
[1]  
ALLER LH, 1968, PLANETARY NEBULAE, P339
[2]  
[Anonymous], 1965, OBSERVATORY, V85, P231
[3]  
CASSINELLI JP, 1969, B AAS, V1, P209
[4]   ON ABSOLUTE MAGNITUDE AND EFFECTIVE TEMPERATURE OF HYDROGEN-POOR STAR HD 30353 [J].
DANZIGER, IJ ;
WALLERST.G ;
BOHMVITE.E .
ASTROPHYSICAL JOURNAL, 1967, 150 (1P1) :239-&
[5]  
DOKUCHAEVA OD, 1976, 1189 INF B VAR STARS
[6]  
FELDMAN PA, 1977, IAU3083 CIRC
[7]  
FELDMAN PA, 1977, IAU3081 CIRC
[8]   POSSIBLE PLANETARY NEBULA [J].
STOVER, RJ ;
SIVERTSEN, S .
ASTROPHYSICAL JOURNAL, 1977, 214 (01) :L33-L34
[9]   SHARP LINES IN THE SPECTRUM OF NOVA RS OPHIUCHI [J].
WALLERSTEIN, G .
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 1958, 70 (417) :537-&