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researcher

Hou-Jun Lu

4 papers here

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author4

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE4
same name
  • Hou-Jun Lu — 31 papers

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20242026
collaborators

4 papers

astro-ph.HE2026

Identifying the poynting-flux-dominated outflow of Fermi GRBs with non-thermal spectrum and its energy-resolved light curve fitting

Xue-Zhao Chang, HouJun Lü, Zhao-Wei Du +2

The jet compositions of gamma-ray bursts (GRBs) are very important to understand the energy dissipation and radiation mechanisms, but it remains an open question in GRB physics. In…

astro-ph.HE2025

How to identify the object with mass range of (2.2−3)M⊙​ 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.HE2024

The thermal emission in short GRBs with extended emission observed by Fermi/GBM

Xue-Zhao Chang, Hou-Jun Lü, Xing Yang +2

Short gamma-ray bursts (SGRBs) with extended emission (EE) are composed of initial main emission (ME) with a short-hard spike, followed by a long-lasting EE. Whether the ME and EE…

astro-ph.HE2024

The X-ray re-brightening of GRB afterglow revisited: a possible signature from activity of the central engine

Zhe Yang, Hou-Jun Lü, Xing Yang +2

Long-duration gamma-ray bursts (GRBs) are thought to be from core collapse of massive stars, and a rapidly spinning magnetar or black hole may be formed as the central engine. The…

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