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Yong Zhang

4 papers hereh-index 4122 citations6 works total

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

author position
  • first author3
  • middle author1

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

fields
  • astro-ph4
same name
  • Yong Zhang — 17 papers, h 13
  • Yong Zhang — 5 papers, h 20
  • Yong Zhang — 3 papers, h 2
  • Yong Zhang — 2 papers, h 24
  • Yong Zhang — 2 papers, h 3
  • Yong Zhang — 2 papers, h 9

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 citedAbundances of s-process elements in planetary nebulae: Br, Kr & Xe

4 citations · 4 across the 1 of their papers we have counts for

collaborators

4 papers

astro-ph2006★ 4 cited

Abundances of s-process elements in planetary nebulae: Br, Kr & Xe

Y. Zhang, R. Williams, E. Pellegrini +5

We identify emission lines of post-iron peak elements in very high signal-to-noise spectra of a sample of planetary nebulae. Analysis of lines from ions of Kr and Xe reveals enhanc…

astro-ph2005

Integrated spectrum of the planetary nebula NGC 7027

Y. Zhang, X. -W. Liu, S. -G. Luo +2

We present deep optical spectra of the archetypal young planetary nebula (PN) NGC 7027, covering a wavelength range from 3310 to 9160 A. The observations were carried out by unifor…

astro-ph2005

Helium recombination spectra as temperature diagnostics for planetary nebulae

Y. Zhang, X. -W. Liu, Y. Liu +1

Electron temperatures derived from the \ion{He}{1} recombination line ratios, designated Te​(\ion{He}{1}), are presented for 48 planetary nebulae (PNe). We study the effect…

astro-ph2004

Observations and 3D photoionisation modelling of the Wolf-Rayet planetary nebula NGC 1501

Barbara Ercolano, R. Wesson, Y. Zhang +4

Deep optical spectra of the high excitation planetary nebula NGC 1501 and its W04 central star are presented. A recombination line abundance analysis of the central star's emission…

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