73 citations
- Tsinghua UniversityCN68 papers
- Chinese Academy of SciencesCN67 papers
- National Astronomical ObservatoriesCN60 papers
- Beijing Academy of Science and TechnologyCN51 papers
- University of Chinese Academy of SciencesCN47 papers
- Yunnan ObservatoriesCN37 papers
- Beijing Normal UniversityCN32 papers
- University of California, BerkeleyUS26 papers
- Tel Aviv UniversityIL19 papers
- Las Cumbres Observatory Global Telescope NetworkUS18 papers
- University of California, Santa BarbaraUS18 papers
- Purple Mountain ObservatoryCN16 papers
14 papers · 2 filters
SN 2019ewu: A Peculiar Supernova with Early Strong Carbon and Weak Oxygen Features from a New Sample of Young SN Ic Spectra
Marc Williamson, Christian Vogl, Maryam Modjaz +17
With the advent of high cadence, all-sky automated surveys, supernovae (SNe) are now discovered closer than ever to their dates of explosion. However, young pre-maximum light follo…
The Interaction of Supernova 2018evt with a Substantial Amount of Circumstellar Matter -- An SN1997cy-like Event
Yi Yang, Dietrich Baade, Peter Hoeflich +29
A rare class of supernovae (SNe) is characterized by strong interaction between the ejecta and several solar masses of circumstellar matter (CSM) as evidenced by strong Balmer-line…
Torque reversals and wind variations of X-ray pulsar Vela X-1
Zhenxuan Liao, Jiren Liu, Lijun Gou
The erratic spin history of Vela X-1 shows some continuous spin-up/spin-down trend over tens of days. We study the orbital profile and spectral property of Vela X-1 in these spin-u…
SN 2019ein: A Type Ia Supernova Likely Originated from a Sub-Chandrasekhar-Mass Explosion
Gaobo Xi, Xiaofeng Wang, Wenxiong Li +12
We present extensive optical photometric and spectroscopic observations for the nearby Type Ia supernova (SN Ia) 2019ein, spanning the phases from days to days…
Comparing the Super-Eddington accretion of SMC X-3 and RX J0209.6-7427 with Swift J0243.6+6124
Jiren Liu, Georgios Vasilopoulos, MingYu Ge +4
We study the giant outbursts of SMC X-3 and RX J0209.6-7427 to compare their super-Eddington accretion regime with that of Swift J0243.6+6124. The high double-peak profile of SMC X…
iPTF14hls in the circumstellar medium interaction model: A promising candidate for a pulsational pair-instability supernova
Ling-Jun Wang, Liang-Duan Liu, Wei-Li Lin +4
iPTF14hls is a luminous Type II supernova (SN) with a bumpy light curve that remains debated for its origin. It maintains roughly a constant effective temperature and luminosity si…