SPEEDY MIC - A VERY YOUNG, RAPIDLY ROTATING K-STAR

被引:17
作者
ANDERS, GJ
JEFFRIES, RD
KELLETT, BJ
COATES, DW
机构
[1] UNIV BIRMINGHAM,SCH PHYS & SPACE RES,BIRMINGHAM B15 2TT,ENGLAND
[2] RUTHERFORD APPLETON LAB,SPACE ASTRON GRP,DIDCOT OX11 0QX,OXON,ENGLAND
关键词
STARS; ABUNDANCES; ACTIVITY; INDIVIDUAL; HD; 197890; LATE-TYPE; PRE-MAIN-SEQUENCE; ROTATION;
D O I
10.1093/mnras/265.4.941
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The active K-type object HD 197890 detected in the ROSAT all-sky survey appears to be one of the most rapidly rotating stars of its type yet found, with a v sin i value of 170 +/- 20 km s(-1). Preliminary photometric measurements and spectral synthesis of the Li 6707-Angstrom spectral region suggest a pre-main-sequence evolutionary status, although the derived spectral type of approximately K5 is uncertain at this stage, and further observations are planned.
引用
收藏
页码:941 / 945
页数:5
相关论文
共 21 条
[1]  
Allen C. W., 1973, ASTROPHYSICAL QUANTI, P206
[2]   EVIDENCE THAT THE ACTIVE STARS HD-102077 (V 838-CEN) AND HD-139084 (V 343-NOR) ARE MEMBERS OF THE LOCAL ASSOCIATION [J].
ANDERS, GJ ;
INNIS, JL ;
COATES, DW ;
THOMPSON, K .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1991, 252 (03) :408-413
[3]   SPOT MODELING OF AB-DOR, 1980-1991 [J].
ANDERS, GJ ;
COATES, DW ;
THOMPSON, K .
PROCEEDINGS ASTRONOMICAL SOCIETY OF AUSTRALIA, 1992, 10 (01) :33-37
[4]  
BASTIAN U, 1990, B INF CTR DONNEES ST, V50, P197
[5]  
Bell R. A., 1976, Astronomy and Astrophysics Supplement Series, V23, P37
[6]  
BROMAGE GE, 1992, ASTR SOC P, V26, P80
[7]  
BROMAGE GE, 1992, ASTR SOC P, V26, P61
[8]  
BROWN A, 1993, UNPUB APJ
[9]  
CHIU HY, 1968, STELLAR PHYSICS, V1, P490