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An interacting O + O supergiant close binary system: Cygnus OB2-5 (V729 Cyg)
Institution:1. Max-Planck-Institut für Sonnensystemforschung (MPS), Justus-von-Liebig-Weg 3, 37077 Göttingen, Germany;2. Dept. of Physics, Indian Institute of Technology (Banaras Hindu University), Varanasi 221005, India;1. Max-Planck-Institut für Sonnensystemforschung (MPS), 37077 Göttingen, Germany;2. Dept. of Physics, Indian Institute of Technology (Banaras Hindu University), Varanasi 221 005, India;1. Chemistry Department, King Fahd University of Petroleum and Minerals, Dhahran 31261, Saudi Arabia;2. Chemistry Department, Faculty of Mathematics and Natural Sciences, Universitas Islam Indonesia, Yogyakarta 55584, Indonesia;1. Department of Chemistry, Sardar Vallabhbhai National Institute of Technology, Surat 395007, Gujarat, India;2. ASPEE SHAKILAM Biotechnology Institute, Navsari Agricultural University, Surat 395007, Gujarat, India;3. Analytical Chemistry Division, Bhabha Atomic Research Center, Trombay, Mumbai 400085, India;1. Department of Medical Services and Techniques, Yunus Emre Vocational School of Health Services, Anadolu University, 26470 Eski?ehir, Turkey;2. Department of Education Lahore, Computer Science and Technology, 54840 Punjab, Pakistan;3. Department of Chemistry and Environmental Science, New Jersey Institute of Technology, Newark, NJ 07102, USA
Abstract:
Keywords:Stars: binaries  Stars: binaries: close  Stars: individual: V729 Cyg  Stars: fundamental parameters  Stars: early-type  Galaxy: open clusters and associations: individual Cygnus OB2
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