Jun Mo

5 та иш

Physics Department and Tsinghua Center for Astrophysics (THCA), Tsinghua University, Beijing, 100084, People’s Republic of China

1. Observations of SN 2017ein Reveal Shock Breakout Emission and a Massive Progenitor Star for a Type Ic Supernova

   Danfeng Xiang, Xiaofeng Wang, Jun Mo +23

   МақолаGamma-ray bursts and supernovaeThe Astrophysical Journal20193 иқтибос

   ABIABI:AkademIndex/openalex/2026.other.117082

2. The Peculiar Transient AT2018cow: A Possible Origin of a Type Ibn/IIn Supernova

   Danfeng Xiang, Xiaofeng Wang, Weili Lin +47

   МақолаGamma-ray bursts and supernovaeThe Astrophysical Journal20211 иқтибос

   ABIABI:AkademIndex/openalex/2021.article.000168

3. SN 2019ein: a Type Ia supernova likely originated from a sub-Chandrasekhar-mass explosion

   Gaobo Xi, Xiaofeng Wang, Wenxiong Li +12

   МақолаGamma-ray bursts and supernovaeMonthly Notices of the Royal Astronomical Society20221 иқтибос

   ABIABI:AkademIndex/openalex/2026.other.252769

4. Optical and ultraviolet monitoring of the black hole X-ray binary MAXI J1820+070/ASASSN-18ey for 18 months

   Hanna Sai, Xiaofeng Wang, Jianfeng Wu +20

   МақолаAstrophysical Phenomena and ObservationsMonthly Notices of the Royal Astronomical Society20210 иқтибос

   ABIABI:AkademIndex/openalex/2021.article.000493

5. A superluminous supernova lightened by collisions with pulsational pair-instability shells

   Weili Lin, Xiaofeng Wang, Lin Yan +23

   МақолаGamma-ray bursts and supernovaeNature Astronomy20230 иқтибос

   ABIABI:AkademIndex/openalex/2023.article.000208