THE DEGREE OF COMPLETENESS OF NEARBY STARS AND THE STELLAR LUMINOSITY FUNCTION

被引:42
作者
UPGREN, AR
ARMANDROFF, TE
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D O I
10.1086/113069
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P1 [天文学];
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0704 ;
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页码:1898 / 1908
页数:11
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共 44 条
[1]  
[Anonymous], MK SPECTRAL CLASSIFI
[2]  
ARAKELYAN MA, 1968, ASTROFIZIKA, V4, P618
[3]   THE UNIVERSE AT FAINT MAGNITUDES .1. MODELS FOR THE GALAXY AND THE PREDICTED STAR COUNTS [J].
BAHCALL, JN ;
SONEIRA, RM .
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 1980, 44 (01) :73-110
[5]   LUMINOSITY LAW FOR LATE-TYPE MAIN-SEQUENCE STARS IN SOLAR NEIGHBORHOOD [J].
EGGEN, OJ .
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 1974, 86 (513) :697-741
[6]  
ELVIUS T, 1965, STARS STELLAR SYSTEM, V5, P41
[7]  
Gliese W., 1979, Astronomy and Astrophysics Supplement Series, V38, P423
[8]  
GLIESE W, 1981, CDS20 B INF
[9]  
GLIESE W, 1971, VEROFF ASTRON I HEID, V24
[10]  
GLIESE W, 1978, IAU S, V80, P79