◍wovepaper
SearchResearchersInstitutions
Sign in
researcher

X. Wu

5 papers hereh-index 202.8k citations46 works total

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

author position
  • middle author4
  • last author1

Across the 5 of 5 papers where every author was matched, so the position is known.

fields
  • astro-ph5
same name
  • X. Wu — 26 papers
  • X. Wu — 11 papers, h 22
  • X. Wu — 2 papers, h 7
  • X. Wu — 1 paper, h 4
  • X. Wu — 1 paper, h 10
  • X. Wu — 1 paper, h 2

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
20032006
collaborators

5 papers

astro-ph2006

Estimation of the detectability of optical orphan afterglows

Y. C. Zou, X. F. Wu, Z. G. Dai

By neglecting sideways expansion of gamma-ray burst (GRB) jets and assuming their half-opening angle distribution, we estimate the detectability of orphan optical afterglows. This…

astro-ph2005

Early Afterglows in Wind Environments Revisited

Y. C. Zou, X. F. Wu, Z. G. Dai

When a cold shell sweeps up the ambient medium, a forward shock and a reverse shock will form. We analyze the reverse-forward shocks in a wind environment, including their dynamics…

astro-ph2005

Testing Gamma-Ray Burst Jet Structure with the Distribution of Gamma-Ray Energy Release

L. Xu, X. F. Wu, Z. G. Dai

We present a general method for testing gamma-ray burst (GRB) jet structure and carry out a comprehensive analysis about the prevalent jet structure models. According to the jet an…

astro-ph2003

Rebrightening of XRF 030723: further evidence for a two-component jet in gamma-ray burst

Y. F. Huang, X. F. Wu, Z. G. Dai +2

Optical afterglows from two-component jets under various configurations are investigated numerically. Generally, the light curve is characterized by a rapid rebrightening when the…

astro-ph2003

GRB 030226 in a Density-Jump Medium

Z. G. Dai, X. F. Wu

We present an explanation for the unusual temporal feature of the GRB 030226 afterglow. The R-band afterglow of this burst faded as ~ t^{-1.2} in ~ 0.2 days after the burst, rebrig…

◍wovepaper

Papers, researchers and institutions, woven together.

Explore
  • Search
  • Researchers
  • Institutions
Account
  • Library
  • Chat
Data
  • arXiv.org
  • Semantic Scholar
  • OpenAlex
  • Latest RSS
AboutContactPrivacyDevelopersllms.txtopenapi.json
Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.