Neutron Star Kicks plus Rockets as a Mechanism for Forming Wide Low-eccentricity Neutron Star Binaries

Recent neutron star surface observations corroborate a long-standing theory that neutron stars may be accelerated over extended periods after their birth. We analyze how these prolonged rocket-like accelerations, combined with rapid birth kicks, impact binary orbits. We find that even a small contri...

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গ্রন্থ-পঞ্জীর বিবরন
প্রধান লেখক: Ryosuke Hirai, Philipp Podsiadlowski, Alexander Heger, Hiroki Nagakura
বিন্যাস: প্রবন্ধ
ভাষা:English
প্রকাশিত: IOP Publishing 2024-01-01
মালা:The Astrophysical Journal Letters
বিষয়গুলি:
অনলাইন ব্যবহার করুন:https://doi.org/10.3847/2041-8213/ad6e77
বিবরন
সংক্ষিপ্ত:Recent neutron star surface observations corroborate a long-standing theory that neutron stars may be accelerated over extended periods after their birth. We analyze how these prolonged rocket-like accelerations, combined with rapid birth kicks, impact binary orbits. We find that even a small contribution of rocket kicks combined with instantaneous natal kicks can allow binaries to reach period–eccentricity combinations unattainable in standard binary evolution models. We propose these kick + rocket combinations as a new channel to form wide low-eccentricity neutron star binaries such as Gaia NS1, as well as inducing stellar mergers months to years after a supernova to cause peculiar high-energy transients.
আইএসএসএন:2041-8205