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• W3044927862 abstract "We performed population synthesis simulations of Population III binary stars with Maxwellian kick velocity distribution when MGCOs (Mass Gap Compact Objects with mass 2--5$,M_{odot}$) are formed. We found that for eight kick velocity dispersion models of $sigma_{rm k}=0$--$500$ km/s, the mean mass of black hole (BH)-MGCO binary is $sim (30 ,M_odot,,2.6 ,M_odot)$. In numerical data of our simulations, we found the existence of BH-MGCO binary with mass $(22.9 ,M_odot,,2.5 ,M_odot)$ which looks like GW190814." @default.
• W3044927862 created "2020-07-29" @default.
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• W3044927862 date "2020-07-27" @default.
• W3044927862 modified "2023-10-01" @default.
• W3044927862 title "Formation of mass gap compact object and black hole binary from Population III stars" @default.
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