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Sheng-Li Qin

4 papers hereh-index 12 citations5 works total

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

author position
  • middle author2
  • last author2

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

fields
  • astro-ph.GA3
  • astro-ph.SR1
same name
  • Sheng-li Qin — 27 papers, h 7
  • Sheng-Li Qin — 3 papers, h 2

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

collaborators

4 papers

astro-ph.GA2026

Interferometric molecular line observations toward the 21 μm protoplanetary nebula IRAS 06530-0213

Hao-Min Sun, Zhuang Zhang, Jun-Yang Liu +2

The identification of the 21μm feature in some protoplanetary nebulae remains a longstanding puzzle, whose interpretation requires characterization of the molecular ga…

astro-ph.GA2026

Herschel/HIFI Observations of Molecular Lines Toward G10.47+0.03

Indrajit Mondal, Prasanta Gorai, Ankan Das +6

We present a spectral line analysis of the hot molecular core G10.47+0.03 (hereafter, G10). Our aim is to determine molecular abundances and excitation conditions across a wide spe…

astro-ph.SR2025

Cocoon-to-Butterfly Transformation in Protoplanetary Nebula: Detection of a Spherical Halo and a Barrel-shaped Torus in IRAS 06530−0213

Hao-Min Sun, Yong Zhang, Sheng-Li Qin

Protoplanetary nebulae (PPNs) represent a critical evolutionary bridging stage between the asymptotic giant branch (AGB) and planetary nebula (PN) stages. Their dynamical structure…

astro-ph.GA2025

A molecule-rich torus-like structure in the 21 μm source IRAS 23304+6147

Hao-Min Sun, Yong Zhang, Xu-Jia Ouyang +4

A long-standing enigma in observational astronomy is the identification of the so-called 21 μm feature in a subset of envelopes of post-asymptotic giant branch (post-AGB) stars.…

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