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Analysis of the massive eclipsing binary V1441 Aql
Affiliation:1. Ege University, Science Faculty, Astronomy and Space Sciences Dept., 35100 Bornova, İzmir, Turkey;2. Osservatorio Astrofisico di Catania, Via S. Sofia 78, 95123 Catania, Italy;1. Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, China;2. Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, China;3. University of Chinese Academy of Sciences, Beijing 100049, China;1. Department of Physics and Astronomy, George Mason University, 4400 University Drive, Fairfax, VA 22030, USA;2. Department of Physics and Astronomy, University of Alabama, 514 University Blvd E, Box 870324, Tuscaloosa, AL 35487, USA;1. Ankara University, Faculty of Science, Department of Astronomy and Space Sciences, TR-06100 Tandoğan, Ankara, Turkey;2. Department of Astronomy and Satellite Geodesy, Kazan Federal University (KFU), 420008 Kazan, Russia;3. Tokyo Institute of Technology, 2-12-1 Ookayama, Meguro-ku, Tokyo 152-8550, Japan;4. Academy of Sciences of Tatarstan, Bauman Str, 20, 420111 Kazan, Russia;5. Ege University, Faculty of Science, Department of Astronomy and Space Sciences, TR-35100 Bornova, İzmir, Turkey;6. Okayama Astrophysical Observatory, National Astronomical Observatory, Honjo 3037-5, Kamogata, Okayama 719-0232, Japan;7. Advanced Technology Center, National Astronomical Observatory, Osawa 2-21-1, Mitaka, Tokyo 181-8588, Japan
Abstract:
Keywords:Stars: binaries: eclipsing  Stars: fundamental parameters  Stars: binaries: spectroscopic
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