Add to ORKGABSTRACT. New differential time-series observations of BL Camelopardalis were secured using B and V filters. It was confirmed that BL Cam is an optical double star. Differential magnitudes were obtained through a photometric profile reduction procedure to eliminate the influence of a faint adjacent star. Variations in valuesO C for light maxima were investigated. We found that the parabolic period variation was recently reversed. The periods of BL Cam were investigated, and five frequencies were determined using Fourier analysis. We also investigated the relationship between metallicities and period ratios, and we compared the theoretical and observational relationships. It was found that the theoretical relationship is better than the obs...
Context.Short-period high-amplitude pulsating stars of Population I (d Sct stars) and II (SX Phe var...
New CCD photometric observations of BXDra were carried out on 26 nights during the period from 2009 ...
The paper is devoted to the problem of the determination of the orbital and physical parameters of ...
Differential time-series observations of BL Camelopardalis classified as a double mode SX Phoenicis ...
We report optical observations of the VY Scl star BZ Cam during its previous optical low state in 1...
New BVR light curves and times of minimum light for the short period RS CVn system SV Cam were analy...
WOS: 000248394400032Context. BL Cam is an extreme metal-deficient field high-amplitude SX Phe-type v...
Context. BL Cam is an extreme metal-deficient field high-amplitude SX Phe-type variable where a very...
Context. BL Cam is an extreme field multiperiodic short-period low-metallicity high-amplitude SX Phe...
Context. BL Cam is an extreme metal-deficient field high-amplitude SX Phe-type variable where a very...
International audienceContext. Short-period high-amplitude pulsating stars of Population I (delta Sc...
We present the optical (V, R, and I) photometry for BL Lacertae, which was observed from 1997 throug...
Astronomy and Astrophysics, v. 451, p. 999-1008, 2006. http://dx.doi.org/10.1051/0004-6361:20053841I...
Radial velocities from 1916.95 to 1991.95 and photometry from 1979.25 to 1992.40, both published and...
Context. Short-period high-amplitude pulsating stars of Population I (delta Sct stars) and II (SX Ph...
Context.Short-period high-amplitude pulsating stars of Population I (d Sct stars) and II (SX Phe var...
New CCD photometric observations of BXDra were carried out on 26 nights during the period from 2009 ...
The paper is devoted to the problem of the determination of the orbital and physical parameters of ...
Differential time-series observations of BL Camelopardalis classified as a double mode SX Phoenicis ...
We report optical observations of the VY Scl star BZ Cam during its previous optical low state in 1...
New BVR light curves and times of minimum light for the short period RS CVn system SV Cam were analy...
WOS: 000248394400032Context. BL Cam is an extreme metal-deficient field high-amplitude SX Phe-type v...
Context. BL Cam is an extreme metal-deficient field high-amplitude SX Phe-type variable where a very...
Context. BL Cam is an extreme field multiperiodic short-period low-metallicity high-amplitude SX Phe...
Context. BL Cam is an extreme metal-deficient field high-amplitude SX Phe-type variable where a very...
International audienceContext. Short-period high-amplitude pulsating stars of Population I (delta Sc...
We present the optical (V, R, and I) photometry for BL Lacertae, which was observed from 1997 throug...
Astronomy and Astrophysics, v. 451, p. 999-1008, 2006. http://dx.doi.org/10.1051/0004-6361:20053841I...
Radial velocities from 1916.95 to 1991.95 and photometry from 1979.25 to 1992.40, both published and...
Context. Short-period high-amplitude pulsating stars of Population I (delta Sct stars) and II (SX Ph...
Context.Short-period high-amplitude pulsating stars of Population I (d Sct stars) and II (SX Phe var...
New CCD photometric observations of BXDra were carried out on 26 nights during the period from 2009 ...
The paper is devoted to the problem of the determination of the orbital and physical parameters of ...