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Zhaojun Wang

28 papers hereh-index 10313 citations50 works total

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

author position
  • first author4
  • middle author17
  • last author6

Across the 27 of 28 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR18
  • astro-ph.HE6
  • astro-ph.GA2
  • astro-ph1
  • gr-qc1
same name
  • Zhaojun Wang — 10 papers, h 3
  • Zhaojun Wang — 8 papers, h 36
  • Zhaojun Wang — 6 papers, h 2
  • Zhaojun Wang — 4 papers, h 14
  • Zhaojun Wang — 3 papers, h 7
  • Zhaojun Wang — 3 papers, h 10

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
20082022
most citedEffects of Irradiation on the Evolution of Ultra-compact X-ray Binaries

24 citations · 213 across the 28 of their papers we have counts for

collaborators
Showing 2013Show all

4 papers · 1 filter

astro-ph.SR2013★ 22 cited

Origin of Dust around V1309 Sco

Chunhua Zhu, Guoliang Lu, Zhaojun Wang

The origin of dust grains in the interstellar medium is still open problem. \cite{Nicholls2013} found the presence of a significant amount of dust around V1309 Sco which maybe orig…

astro-ph.SR2013★ 12 cited

Low-mass X-ray Binaries with Strange Quark Stars

Chunhua Zhu, Guoliang Lv, Zhaojun Wang +1

Strange quark stars (SSs) may originate from accreting neutron stars (NSs) in low-mass X-ray binaries (LMXBs). Assuming that conversion of NS matter to SSs occurs when the core den…

astro-ph.SR2013★ 8 cited

Donors of Persistent Neutron-star Low-mass X-ray Binaries

Chunhua Zhu, Guoiliang Lv, Zhaojun Wang +1

Properties of X-ray luminosities in low-mass X-ray binaries (LMXBs) mainly depend on donors. We have carried out a detailed study of donors in persistent neutron-star LMXBs (PLMXBs…

astro-ph.SR2013★ 6 cited

The Shoenberg Effect in Relativistic Degenerate Electron Gas and Observational Evidences in Magnetars

Zhaojun Wang, Guoliang Lv, Chunhua Zhu +1

The electron gas inside a neutron star is highly degenerate and relativistic. Due to the electron-electron magnetic interaction, the differential susceptibility can equal or exceed…

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