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researcher

Jing Wen

3 papers here

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

author position
  • first author2
  • last author1

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR2
  • astro-ph.GA1
ORCID 0000-0002-0034-3391
same name
  • Jing Wen — 1 paper, h 18
  • Jing Wen — 1 paper, h 0
  • Jing Wen — 1 paper
  • Jing Wen — 1 paper
  • Jing Wen — 1 paper
  • Jing Wen — 1 paper

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

3 papers

astro-ph.SR2024

Mass-loss Rate of Highly Evolved Stars in the Magellanic Clouds

Jing Wen, Ming Yang, Jian Gao +3

Asymptotic giant branch stars (AGBs) and red supergiant stars (RSGs) exhibit significant mass loss phenomena and are considered important sources of interstellar dust. In this work…

astro-ph.SR2024

Evolved Massive Stars at Low-metallicity VII. the Lower Mass Limit of Red Supergiant Population in the Large Magellanic Cloud

Ming Yang, Bo Zhang, Biwei Jiang +8

The precise definition of the lower mass limit of red supergiant stars (RSGs) is an open question in astrophysics and does not attract too much attention. Here we assemble a spectr…

astro-ph.GA2024

Evolved Massive Stars at Low-metallicity VI. Mass-Loss Rate of Red Supergiant Stars in the Large Magellanic Cloud

Jing Wen, Jian Gao, Ming Yang +4

Mass loss is a crucial process that affects the observational properties, evolution path and fate of highly evolved stars. However, the mechanism of mass loss is still unclear, and…

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