A period investigation of two chromospherically active binary stars: RT Coronae Borealis and PW Herculis

• المؤلفون الرئيسيون: Qian S.B., Zhu L.Y., He J.J., Boonruksar S.
• التنسيق: مقال
• اللغة: English
• منشور في: 2014
• الوصول للمادة أونلاين: http://www.scopus.com/inward/record.url?eid=2-s2.0-0037810645&partnerID=40&md5=1a40de57e4ccc87dda584f331e9fc3a9; http://cmuir.cmu.ac.th/handle/6653943832/6037
• المؤسسة: Chiang Mai University

Orbital period variations of two chromospherically active binary systems, RT CrB and PW Her, are presented. It is shown that the orbital period of RT CrB undergoes a cyclic oscillation with a period of 53.9years. For PW Her, an alternate change, with a period of 42.7years, is found to superimpose on...