Light and colour curve observations and analysis of the short period eclipsing binary system UV Psc |
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Authors: | Sadik Aziz R |
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Institution: | (1) Astronomy Department, Manchester University, England;(2) Present address: Astronomical Observatory Unit, Scientific Research Foundation, Jadiriyah, P.O.B. 255, Baghdad, Iraq |
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Abstract: | In the present work we have presented and analysedB andV light curves and the (B-V)-colour curve of the short period (RS CVn type) binary system UV Psc, and derived absolute information from the available data.x
2 minimization procedures were utilized to a large extent in fitting light and colour curves.The solutions show the binary to be at a distance of about 90 pc with two detached components which are close to the main sequence (G2 and K0). The inclination of the orbit is close to 90°Photometric irregularities present in the light curve are briefly considered in relation to current ideas on RS CVn systems, and the colour information indicates a locally hotter (rather than cooler) region is responsible for the irregularities. |
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