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Synchrotron emission model of gamma-ray pulsar PSR J2021+3651
Affiliation:1. Center for Theoretical Astrophysics, ITP, Ilia State University, 0162 Tbilisi, Georgia;2. Dublin Institute for Advanced Studies, Fitzwilliam Place., 31, Dublin 2, Ireland;3. Dublin City University, Dublin 9, Ireland;4. Main Astronomical Observatory of NAS of Ukraine, Zabolotnogo str., 27, 03680 Kyiv, Ukraine;1. Indian Centre For Space Physics, 43 Chalantika, Garia Station Road, Kolkata 700084, India;2. S.N. Bose National Center for Basic Sciences, JD-Block, Salt Lake, Kolkata 700098, India;1. Astronomy Department, National Research Institute of Astronomy and Geophysics, 11421 Helwan, Cairo, Egypt;2. Physics Department, College of Science, Northern Border University, 1321 Arar, Saudi Arabia;3. 1393 Garvin Street, Prince George, BC V2M 3Z1, Canada;1. College of Science/Department of Physics & NAOC-GZU-Sponsored Center for Astronomy Research, Guizhou University, Guiyang 550025, PR China;2. Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650011, PR China;3. Dept. of Physics and Astronomy, Butler University, Indianapolis, IN 46208, USA;4. Bundesdeutsche Arbeitsgemeinschaft für Veränderliche Sterne e.V.(BAV), Munsterdamm 90, D-12169 Berlin, Germany;1. Departament d’Arquitectura i Tecnologia de Computadors, Universitat de Girona, Spain;2. Departamento de Física, Universidad de Jaén, Spain;3. Departament d’Astronomia i Meteorologia and Institut de Ciències del Cosmos, Universitat de Barcelona, Spain;1. Ankara University, Science Faculty, Dept. of Astronomy and Space Sciences, 06100 Tandoğan, Ankara, Turkey;2. Eastern University, Dept. of Astronomy & Physics, St. Davids, PA 19087, USA
Abstract:
Keywords:(Stars:) pulsars: individual PSR J2021+3651  Stars: magnetic fields  Radiation mechanisms: non-thermal
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