MAGNETIC-STRUCTURE IN COOL STARS .15. THE EVOLUTION OF ROTATION RATES AND CHROMOSPHERIC ACTIVITY OF GIANTS

被引：0

作者：

RUTTEN, RGM ^{[1
]}

PYLYSER, E ^{[1
]}

机构：

[1] STERRENKUNDIG INST ANTON PANNEKOEK, 1018 WB AMSTERDAM, NETHERLANDS

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中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：227 / 236

页数：10

共 65 条

ALSCHULER, WR .

[2]

[Anonymous], REVISED CATALOGUE ST

[3] THE COOL HALF OF THE H-R DIAGRAM IN SOFT X-RAYS [J].

AYRES, TR ;

LINSKY, JL ;

VAIANA, GS ;

GOLUB, L ;

ROSNER, R .

[4]

BENZ W, 1981, ASTRON ASTROPHYS, V93, P235

[5]

BERNACCA PL, 1970, CONTR OSS ASTROFIS P, V239

[6]

BERNACCA PL, 1973, CONTR OSS ASTROFIS P, V294

[7]

BIANCHI L, 1985, ASTRON ASTROPHYS, V149, P41

[8] THE EFFECTIVE TEMPERATURE SCALE [J].

BOHMVITENSE, E .

[9]

CATALANO S, 1983, ASTRON ASTROPHYS, V121, P190

[10]

COHEN JG, 1972, ASTROPHYS J, V171, P71, DOI 10.1086/151259