VARIABILITY OF STARS IN THE PRIMARY STANDARD GROUP FOR THE WBVR PHOTOMETRIC SYSTEM

被引：0

作者：

KUSAKIN, AV

MIRONOV, AV

MOSHKALEV, VG

机构：

来源：

SOVIET ASTRONOMY LETTERS | 1991年 / 17卷 / 02期

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The magnitude of four standard stars for the WBVR photometric system has been reinvestigated. The constancy of the magnitude of HD 221525 and HD 224687 is confirmed. The star HD 221142 turns out to be a delta-Scuti variable with a period 0.0729638 days and an amplitude 0m.023 in the V band. The star HD 221829 turns out to be a variable of the Ell type with a period 0.4851142 days and an approximate amplitude 0m.020 in all bands.

引用

页码：110 / 113

页数：4