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Wei Wang

4 papers hereh-index 4121 citations5 works total

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

author position
  • sole author1
  • first author1
  • last author2

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

fields
  • astro-ph4
same name
  • Wei Wang — 349 papers
  • Wei Wang — 102 papers, h 34
  • Wei Wang — 63 papers, h 53
  • Wei Wang — 42 papers, h 8
  • Wei Wang — 36 papers, h 14
  • Wei Wang — 35 papers, h 55

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
20042006
most citedPulsar Wind Nebulae and the X-Ray Emission of Non-Accreting Neutron Stars

58 citations · 129 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph2006★ 38 cited

Pulsar Wind Nebulae and the Non-thermal X-Ray Emission of Millisecond Pulsars

K. S. Cheng, Ronald E. Taam, W. Wang

The non-thermal, non-pulsed X-ray emission of MSPs is investigated. As in young pulsars, MSPs emit a relativistic wind, which interacting with the interstellar medium and/or a bina…

astro-ph2005

Millisecond pulsar population in the Galactic center and high energy contributions

W. Wang

We propose that there possibly exists a population of millisecond pulsars in the Galactic center region. Millisecond pulsars (MSPs) could emit GeV gamma-rays through synchrotron-cu…

astro-ph2005★ 33 cited

Contribution to diffuse gamma-rays in the Galactic center region from unresolved millisecond pulsars

W. Wang, Z. J. Jiang, K. S. Cheng

The diffuse gamma-rays in the Galactic center region have been studied. We propose that there exists a population of millisecond pulsars (MSPs) in the Galactic Center, which will e…

astro-ph2004★ 58 cited

Pulsar Wind Nebulae and the X-Ray Emission of Non-Accreting Neutron Stars

K. S. Cheng, Ronald E. Taam, W. Wang

The general properties of the non-thermal non-pulsed X-ray emission of rotation powered pulsars are investigated in the context of a pulsar wind nebula model. An examination of the…

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