THE PHOTOMETRIC VARIABILITY OF K-GIANTS

被引：16

作者：

PERCY, JR

机构：

来源：

PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC | 1993年 / 105卷 / 694期

关键词：

D O I：

10.1086/133324

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We have photometrically monitored 49 of the more than 200 K giants in the Yale Catalog of Bright Stars which are named or suspected variable stars. Only two (HR 3275 and HR 5219) are clearly variable; a few more program stars and K- and M-giant comparison stars are marginally variable. Most of these appear to be RS Canum Venaticorum or SR variables.

引用

页码：1422 / 1426

页数：5

共 14 条

[1]

CASAS R, 1989, IAU INF B VAR STARS, V3337, P1

[2]

Glebocki R., 1980, Acta Astronomica, V30, P453

[3]

HALBEDEL EM, 1989, IAU INF B VAR STARS, P3394

[4]

HELBEDEL EM, 1993, IAU INF B VAR STARS, P3851

[5]

Hoffleit D., 1982, BRIGHT STAR CATALOG, V4th ed.

[6]

KHOLOPOV PN, 1982, NEW CATALOG SUSPECTE

[7]

KRISCIUNAS K, 1993, DELTA SCUTI STAR NEW, P23

[8]

KUKARKIN BV, 1951, CATALOG SUSPECTED VA

[9]

MAEDER A, 1980, ASTRON ASTROPHYS, V90, P311

[10]

Percy J. R., 1985, Journal of the American Association of Variable Star Observers, V14, P52

← 1 2 →