CL Eri, CM Eri, CN Eri BVIc light curves (Berdnikov+, 2011)

Details CL Eri, CM Eri, CN Eri BVIc light curves (Berdnikov+, 2011) CL Eri, CM Eri, CN Eri BVIc light curves (Berdnikov+, 2011)

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012ycatp004013101b&link_type=abstract

VizieR On-line Data Catalog: J/other/Obs/131.315. Originally published in: 2011Obs...131..315B

Other

Stars: Variable, Photometry: Ubvri, Photometry: Ccd

Scientific paper

A total of total of 1071 B, V, Ic-band CCD frames are 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-10XME. The inferred periods and light-curves confirm that CL Eri (P=0.644d), which was found to exhibit the Blazhko effect, and CN Eri (P=0.580d) are RR Lyr-type variables. CM Eri is most probably a Population-Il Cepheid with a period of 0.824d.
(1 data file).

Affiliated with

Also associated with

No associations

Rating

CL Eri, CM Eri, CN Eri BVIc light curves (Berdnikov+, 2011) does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with CL Eri, CM Eri, CN Eri BVIc light curves (Berdnikov+, 2011), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and CL Eri, CM Eri, CN Eri BVIc light curves (Berdnikov+, 2011) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1643649