The BV Photometry of the RR Lyrae Star, BH Ursae Majoris: Light Curves and Period Study

The first presented BV light curves of BH UMa confirmed Krajci’s (2005) result that BH UMa is an RR Lyr star that belongs to the RRc subgroup. The light curves showed a slight asymmetry of D = 0.453 with an amplitude of about 0.m58 in B, 0.m47 in V, and 0.m11 in B-V and with a small hump between 0...

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Bibliographic Details
Main Authors: Chun-Hwey Kim, Jang Hae Jeong
Format: Article
Language:English
Published: Korean Space Science Society (KSSS) 2011-06-01
Series:Journal of Astronomy and Space Sciences
Subjects:
Online Access:http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2011/v28n2/OJOOBS_2011_v28n2_109.pdf