Full text version of this article in PostScript (600dpi) format compressed by gzip; or in PDF.
Abstract: In this study, an eclipsing binary of a short orbital period (P = 1.d1834857) LV CMa (V = 8.m7) is selected as a candidate member of an association in the direction of CMa OB1/R1 region. Light curves in UBVRcIc photometric bands were obtained and low-resolution (R ∼ 5500) spectra were collected. Preliminary results show that the system is a detached binary containing at least one B spectral type star. It seems that LV CMa has no connection with the nearby OB associations or stellar clusters.
Full text version of this article in PostScript (600dpi) format compressed by gzip; or in PDF.
Last update: May 30, 2019