Period change investigation of the low mass ratio contact binary BO Ari

• Main Authors: W. Kriwattanawong, O. Tasuya, P. Poojon
• Format: Journal
• Published: 2018
• Subjects: Earth and Planetary Sciences; Physics and Astronomy
• Online Access: https://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=84943373953&origin=inward; http://cmuir.cmu.ac.th/jspui/handle/6653943832/55651
• Institution: Chiang Mai University

© 201 5Elsevier B.V. All rights reserved. A photometric study and period change analysis for the A-type low mass ratio contact binary BO Ari is presented. The BVR light curves were fitted by using the Wilson-Devinney method. The photometric solution yields a low mass ratio of q = 0.1754(±0.0016) with a contact degree of f = 27.72%(±2.37%). We found a long-term orbital period decrease at a rate of dPdt=-3.49×10-7d yr-1. This result indicates that the system is undergoing mass transfer from the primary component to the secondary with a mass transfer rate of m1m1= -7.77×10-8yr-1. With the period decrease, the inner and outer critical Roche surfaces will tighten and cause the degree of contact to increase. Therefore, BO Ari may evolve into a deeper contact system.