z-logo
open-access-imgOpen Access
A STUDY OF THE SX PHE STAR BL CAM
Author(s) -
J. H. Peña,
Juan Diego García Paredes,
D. S. Piña,
H. Huepa,
J. Guillén
Publication year - 2021
Publication title -
revista mexicana de astronomía y astrofísica
Language(s) - English
Resource type - Journals
ISSN - 0185-1101
DOI - 10.22201/ia.01851101p.2021.57.02.14
Subject(s) - physics , metallicity , photometry (optics) , astrophysics , star (game theory) , photoelectric effect , binary star , astronomy , stars , optics
We determined the physical parameters of the SX Phe star BL Cam from newly available times of maximum light and other times from the literature, as well as from uvby − β photoelectric photometry. From our analysis we found that this star is a binary system. The mass of the companion star was calculated in term of the mass of the primary star and the orbital angle. For this star we determined a metallicity [Fe/H] of −1.2 ± 0.3.

The content you want is available to Zendy users.

Already have an account? Click here to sign in.
Having issues? You can contact us here