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Z. Wang

4 papers here

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

fields
  • astro-ph4
same name
  • Z. Wang — 9 papers
  • Z. Wang — 8 papers, h 12
  • Z. Wang — 6 papers
  • Z. Wang — 5 papers
  • Z. Wang — 3 papers, h 10
  • Z. Wang — 3 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

most citedSupernova explosions and the birth of neutron stars

14 citations · 20 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph2007★ 2 cited

Suzaku Observation of AXP 1E 1841-045 in SNR Kes 73

M. Morii, S. Kitamoto, N. Shibazaki +7

Anomalous X-ray pulsars (AXPs) are thought to be magnetars, which are neutron stars with ultra strong magnetic field of 1014-- 1015 G. Their energy spectra below ∼10…

astro-ph2007★ 14 cited

Supernova explosions and the birth of neutron stars

H. -Th. Janka, A. Marek, B. Mueller +1

We report here on recent progress in understanding the birth conditions of neutron stars and the way how supernovae explode. More sophisticated numerical models have led to the dis…

astro-ph2007★ 3 cited

Implications of kHz QPOs for the spin frequencies and magnetic fields of neutron stars: new results from Circinus X-1

Stratos Boutloukos, Frederick K. Lamb

Detection of paired kilohertz quasi-periodic oscillations (kHz QPOs) in the X-ray emission of a compact object is compelling evidence that the object is an accreting neutron star.…

astro-ph2007★ 1 cited

The Long-term Radiative Evolution of Anomalous X-ray Pulsar 1E 2259+586 after its 2002 Outburst

Weiwei Zhu, Victoria M. Kaspi, Peter M. Woods +3

We present an analysis of five X-ray Multi-Mirror Mission (XMM) observations of the anomalous X-ray pulsar (AXP) 1E 2259+586 taken in 2004 and 2005 during its relaxation following…

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