...
首页> 外文期刊>Observatory >CCD OBSERVATIONS OF THREE RR LYRAE-TYPE STARS: CL ERI, CM ERI, AND CN ERI
【24h】

CCD OBSERVATIONS OF THREE RR LYRAE-TYPE STARS: CL ERI, CM ERI, AND CN ERI

机译:三颗RR莱拉星型恒星的CCD观测:CL ERI,CM ERI和CN ERI

获取原文
获取原文并翻译 | 示例
           

摘要

A total of 1072 B, V, and I_c-band CCD frames have been taken for three GCVS RR Lyr-type variables (CL Eri, CM Eri, and CN Eri), for which only coordinates were known. Observations were made with the 76-cm telescope of the South African Astronomical Observatory using an SBIG CCD ST-ioXME. The inferred periods and light-curves confirm that CL Eri (P = O~d-644), which was found to exhibit the Blazhko effect, and CN Eri (P = o~d-580) are RR Lyr-type variables. CM Eri is most probably a Population-II Cepheid with a period of o~d.824.
机译:对于三个GCVS RR Lyr类型的变量(CL Eri,CM Eri和CN Eri),总共拍摄了1072 B,V和I_c波段CCD帧,其坐标只有已知。使用SBIG CCD ST-ioXME用南非天文台的76厘米望远镜进行了观测。推定的周期和光曲线证实,发现具有布拉兹科效应的CL Eri(P = O〜d-644)和CN Eri(P = o〜d-580)是RR Lyr型变量。 CM Eri最有可能是一个II期人口造父变星,时期约为824。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号