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BD +14°5016 - A NEW EW ECLIPSING BINARY
Maciejewski, G., Karska, A., Niedzielski, A.
December 3, 2002

BD +14°5016 was found to be variable during the Semi-Automatic Variability Search program at the Piwnice Observatory. The presented photometric data were collected in both B and V filters, during 16 moonless nights between September and November 2002. 334 individual measurements of brightness were made, 275 in V band and 59 in B. The shape of the phased light curve indicates variability of the W UMa type.

According to SIMBAD, BD +14°5016 is a V=9.50 magnitude star of F2 spectral type, with B-V=0.31 mag. Our observations show that at the maximum light the star reaches mV=9.28 mag and mB=9.63 mag. The primary and secondary minima have an amplitude of 0.47 mag and 0.41 mag respectively. The observed amplitudes in B are identical. No noticeable colour variation with phase was detected. The phase-averaged (mB-mV)=0.35. The maximum following the second minimum is 0.04 mag fainter in both bands suggesting presence of a spot placed on the surface of one of the components.


mV, mB and colour curves obtained for BD +14°5016

The period was found with the ANOVA method. The times of both minima were computed from the presented light-curve with the Kwee-van Woerden method. A preliminary ephemeris for the primary minimum is:

Min.I = HJD 2452558.1703(3) + 0.d636889(4) x E. [1]

The shape of the phased light curve clearly shows that the secondary minimum is located at phase 0.52. This fact is confirmed by large O-C values calculated from equation [1] for the observed secondary minima. Therefore the following ephemeris for the secondary minimum has been obtained:

Min.II = HJD 2452557.8658(6) + 0.d636889(4) x E. [2]

To estimate accuracy of calculated minima the collected data were divided in three sessions separated by full moon nights or a long period of bad weather conditions and for each session individual times of minima were determined by the digital tracing paper method. The O-C values, presented below, were calculated for primary and secondary minima from equation [1] and [2] respectively.

Min. HJD Error Type Filter O-C [day]
2452534.2999 0.0014 II V -0.0010
2452534.6031 0.0008 I V -0.0016
2452552.7715 0.0013 II V +0.0008
2452553.073 0.003 I V -0.0024
2452582.706 0.002 II V +0.0014
2452583.007 0.002 I V -0.0014
2452583.3386 0.0032 II B -0.0028
2452583.6441 0.0011 I B -0.0018

The results were published in IBVS 5343 (compressed PostScript). The data are available upon request.

 

Last modified: December 3, 2002.