K EMISSION-LINE WIDTHS IN SUN AND STARS

被引:7
作者
BAPPU, MKV [1 ]
SIVARAMAN, KR [1 ]
机构
[1] INDIAN INST ASTROPHYS,KODAIKANAL 624103,INDIA
关键词
D O I
10.1093/mnras/178.2.279
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
引用
收藏
页码:279 / 287
页数:9
相关论文
共 12 条
[1]   K EMISSION-LINE WIDTHS AND SOLAR CHROMOSPHERE [J].
BAPPU, MK ;
SIVARAMAN, KR .
SOLAR PHYSICS, 1971, 17 (02) :316-+
[2]   THE SOURCE FUNCTION IN A NON-EQUILIBRIUM ATMOSPHERE .5. CHARACTER OF THE SELF-REVERSED EMISSION CORES OF CA+ H AND K [J].
JEFFERIES, JT ;
THOMAS, RN .
ASTROPHYSICAL JOURNAL, 1960, 131 (03) :695-704
[3]   ON RELATIVE RESIDUAL INTENSITIES OF CALCIUM H-LINES AND KILINES [J].
LINSKY, JL .
SOLAR PHYSICS, 1970, 11 (03) :355-&
[4]   MEASUREMENT OF K-LINE ABSOLUTE MAGNITUDES [J].
LUTZ, TE .
ASTRONOMICAL JOURNAL, 1970, 75 (09) :1007-&
[5]   IS SUN A MAGNETIC ROTATOR [J].
SEVERNY, A .
NATURE, 1969, 224 (5214) :53-&
[6]   CA II K EMISSION IN SOUTHERN LATE-TYPE STARS [J].
WARNER, B .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1969, 144 (03) :333-&
[7]   ABSOLUTE MAGNITUDES OF STARS FROM WIDTHS OF CHROMOSPHERIC CA II EMISSION-LINES [J].
WILSON, OC .
ASTROPHYSICAL JOURNAL, 1976, 205 (03) :823-840
[8]   H-EMISSION AND K-EMISSION IN LATE-TYPE STARS - DEPENDENCE OF LINE WIDTH ON LUMINOSITY AND RELATED TOPICS [J].
WILSON, OC ;
BAPPU, MKV .
ASTROPHYSICAL JOURNAL, 1957, 125 (03) :661-&