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Stability of P-type orbits around stellar binaries: An extension to counter-rotating orbits
Affiliation:1. CHEA-SRC, School of Natural Science Ulsan National Institute of Science and Technology (UNIST), Eonyang-eup, Ulju-gun, Ulsan 44919, Republic of Korea;2. Astronomy and Physics, University of Sejong, 209 Neungdong-ro, Gwangjin-gu. Seoul 143-747, Eonyang-eup, Ulju-gun, Ulsan 44919, Republic of Korea;1. Department of Applied Sciences, National Textile University, Faisalabad 37610, Pakistan;2. Department of Mathematics,University of the Punjab, Quaid-i-Azam Campus, Lahore 54590, Pakistan;1. Department of Astronomy, Nanjing University, Nanjing 210023, China;2. Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University), Ministry of Education, China;3. School of Mathematics and Physics, Hebei University of Engineering, Handan 056005, China;1. Department of Physics and Astronomy, Sejong University, Gwangjin-gu, Seoul 143-747, Republic of Korea;2. Istituto Nazionale di Astrofisica Osservatorio Astronomico di Capodimonte, Salita Moiariello 16, Napoli 80131, Italy;3. International Center for Relativistic Astrophysics, Piazzale della Repubblica 2, Pescara 65122, Italy;1. Department of Physics, Technion, Haifa, 3200003, Israel;2. Guangdong Technion Israel Institute of Technology, Shantou 515069, Guangdong Province, China
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