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Shiwei Wu

3 papers hereh-index 356 citations7 works total

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

author position
  • first author3

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA1
  • astro-ph.HE1
  • astro-ph.SR1
same name
  • Shiwei Wu — 16 papers, h 31
  • Shiwei Wu — 13 papers, h 10
  • Shiwei Wu — 8 papers, h 4
  • Shiwei Wu — 6 papers, h 5
  • Shiwei Wu — 5 papers, h 3
  • Shiwei Wu — 4 papers, h 4

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
20112016
most citedGamma-Ray Bursts: the Isotropic-Equivalent-Energy Function and the Cosmic Formation Rate

31 citations · 65 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.GA2016★ 16 cited

The Massive Stellar Population of W49: A Spectroscopic Survey

Shi-Wei Wu, Arjan Bik, Joachim M. Bestenlehner +4

Massive stars form on different scales ranging from large, dispersed OB associations to compact, dense starburst clusters. The complex structure of regions of massive star formatio…

astro-ph.SR2014★ 18 cited

The Discovery of a Very Massive Star in W49

Shi-Wei Wu, Arjan Bik, Thomas Henning +3

Very massive stars (M>100 M⊙​) are very rare objects, but have a strong influence on their environment. The formation of this kind of objects is of prime importance in star…

astro-ph.HE2011★ 31 cited

Gamma-Ray Bursts: the Isotropic-Equivalent-Energy Function and the Cosmic Formation Rate

Shi-Wei Wu, Dong Xu, Fu-Wen Zhang +1

Gamma-ray bursts (GRBs) are brief but intense emission of soft γ−rays, mostly lasting from a few seconds to a few thousand seconds. For such kind of high energy transients, their…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.