摘要
CCD photometric observations of the eclipsing binary PS Persei （PS Per） were obtained on two consecutive days in 2009.The 2003 version of the WilsonDevinney code was used to analyze the first complete light curves in the V and R bands.It is found that PS Per is a short-period Algol-type binary with the less massive component completely filling its inner critical Roche lobe.The mass ratio of q=0.518 and the orbital inclination of i=89.86° are obtained.In addition,based on all available times of primary light minima,including two new ones,the orbital period has been improved.
CCD photometric observations of the eclipsing binary PS Persei （PS Per） were obtained on two consecutive days in 2009.The 2003 version of the WilsonDevinney code was used to analyze the first complete light curves in the V and R bands.It is found that PS Per is a short-period Algol-type binary with the less massive component completely filling its inner critical Roche lobe.The mass ratio of q=0.518 and the orbital inclination of i=89.86° are obtained.In addition,based on all available times of primary light minima,including two new ones,the orbital period has been improved.
基金
supported by the Natural Science Foundation of Shanxi Normal University (No.ZR09002)
