Мақаланы E-mail арқылы жіберу Low-Mass Neutron Stars with Rotation
- Авторлар: Yudin A.V.1,2, Razinkova T.L.1, Blinnikov S.I.1,3
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Мекемелер:
- Institute for Theoretical and Experimental Physics
- “Kurchatov Institute” National Research Center
- Kavli IPMU
- Шығарылым: Том 45, № 12 (2019)
- Беттер: 847-854
- Бөлім: Article
- URL: https://ogarev-online.ru/1063-7737/article/view/191725
- DOI: https://doi.org/10.1134/S1063773719120077
- ID: 191725
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Аннотация
The properties of low-mass neutron stars with rigid rotation are considered. The possible evolution paths of such stars in a close binary system with mass transfer are calculated. The properties of the gamma-ray burst GRB 170817A interpreted in terms of the stripping model, a natural ingredient of which is the explosion of a low-mass neutron star—a binary component, are briefly discussed.
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Авторлар туралы
A. Yudin
Institute for Theoretical and Experimental Physics; “Kurchatov Institute” National Research Center
Хат алмасуға жауапты Автор.
Email: yudin@itep.ru
Ресей, ul. Bolshaya Cheremushkinskaya 25, Moscow, 117259; pl. Kurchatova 1, Moscow, 123182
T. Razinkova
Institute for Theoretical and Experimental Physics
Email: yudin@itep.ru
Ресей, ul. Bolshaya Cheremushkinskaya 25, Moscow, 117259
S. Blinnikov
Institute for Theoretical and Experimental Physics; Kavli IPMU
Email: yudin@itep.ru
Ресей, ul. Bolshaya Cheremushkinskaya 25, Moscow, 117259; Kashiwa
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