Photometric and Spectroscopic Analysis of the SX Phe Star BL Cam

• Published in: Astrophysics 2022-12, Vol.65 (4), p.456-469
• Main Authors: Abdel-Sabour, M., Nouh, M. I., Shokry, A., Hamed, G. M., Ismail, H. A., Takey, A., Ata, S. A., Zead, I.
• Format: Article
• Language: English
• Subjects: Analysis; Astronomy; Astrophysics; Astrophysics and Astroparticles; Astrophysics and Cosmology; Celestial bodies; Computer-aided manufacturing; Fourier analysis; Light curve; Luminosity; Observations and Techniques; Photometry; Physics; Physics and Astronomy; Space Exploration and Astronautics; Space Sciences (including Extraterrestrial Physics; Spectroscopic analysis; Spectroscopic observation; Stars
• ISSN: 0571-7256; 1573-8191
• DOI: 10.1007/s10511-023-09754-6

In the present paper, we report the photometric and spectroscopic observations of the pulsating star BL Cam obtained by the 1.88 m telescope at the Kottamia astronomical observatory (KAO). Fourier analysis of the light curves indicates one frequency, 25.14427 c/d, with harmonics 51.112 c/d, 33.388 c/d, and 17.72464 c/d. The frequency of 31-32 c/d reported in the literature is not detected in our data except for one close to 33.3882934 c/d. A total of 55 new times of maximum light have been presented. A new value of (1/P) dP/dt is estimated using the O-C diagram based on all newly obtained times of maximum light combined with those taken from the literature, assuming the periods are decreasing and changing smoothly. Using model atmosphere analysis, we computed the effective temperature and surface gravity as T eff = 7625 ± 300 K and logg = 4.30 ± 0.37. The bolometric magnitude M bol = 2.335, radius R = 1.69 R ⨀ , luminosity L = 0.957 L ⨀ , the mass M = 1.68M ⨀ , and pulsation constant Q = 0.025 days. Locations of the star on the M-R and M-L diagrams indicate that it is close to the ZAMS track and is an unevolved star.