activity
20242026
collaborators

6 papers

astro-ph.GA2026

B-field Orion Protostellar Survey (BOPS). IV: The Relative Orientation Between Magnetic Fields and Density Structures in Young Protostellar Envelopes

Kexin Cai, Bo Huang, Josep Miquel Girart +7

We investigate the relative alignment between density structures and magnetic fields in eight young protostars from the ALMA B-field Orion Protostellar Survey. Column density maps…

astro-ph.HE2026

The Physical Properties of PS1-12sk and the implications for its Progenitor System

Kai-Li Mi, Shan-Qin Wang, Wen-Pei Gan +3

PS1-12sk is a type Ibn supernova (SN) found in a host environment showing no obvious ongoing star formation, which challenges the massive star explosion scenario. We use the ejecta…

astro-ph.HE2025

The radiative subpulse modulation and spectral features of PSR B192910 with the whole pulse phase emission

Zhengli Wang, Jiguang Lu, Weiyang Wang +7

In this work, we observe the nearby pulsar, PSR B192910, using the Five-hundred-meter Aperture Spherical radio Telescope (FAST). We find, for the first time, two new emission co…

astro-ph.HE2025

How to identify the object with mass range of in the merger of compact star systems

ZhaoWei Du, HouJun Lü, Xiaoxuan Liu +2

High-frequency gravitational-wave (GW) radiation has been detected by LIGO-Virgo-KAGRA in the merger of compact stars. However, two GW events, GW190814 and GW200210, the mass of on…

astro-ph.HE2025

Signature of strange star as the central engine of GRB 240529A

Xiao Tian, HouJun Lü, WenJun Tan +6

GRB 240529A is a long-duration gamma-ray burst (GRB) whose light curve of prompt emission is composed of a triple-episode structure, separated by quiescent gaps of tens to hundreds…

astro-ph.HE2024

An Extreme Radio Fluctuation of Pulsar B192910

Zhengli Wang, Shunshun Cao, Jiguang Lu +7

We report the detection of an extreme flux decrease accompanied by clear dispersion measure (DM) and rotation measure (RM) variations for pulsar B1929+10 during the 110-minute radi…