UBV(RI)C OBSERVATIONS FOR 13 BRIGHT CEPHEIDS

被引：26
|
作者：
SHOBBROOK, RR
机构：
[1] Chatterton Astronomy Department, School of Physics, University of Sydney, 2006, NSW
来源：
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1992年 / 255卷 / 03期
关键词：
D O I：
10.1093/mnras/255.3.486
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Photometry in the UBV(RI)c system has been obtained for 13 of the brightest Cepheids in the southern sky available to the new Sydney University Stellar Interferometer (SUSI). The stars observed were eta Aql, l Car, U Car, AX Cir, beta Dor, zeta Gem, T Mon, kappa Pav, U Sgr, W Sgr, X Sgr, Y Sgr and AH Vel. The main purpose of the photometry is to provide current epoch data for the phases of the variables, although for several of the stars these data are also the first in the (RI)c system.
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页码：486 / 494
页数：9
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