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researcher

Yue Cao

4 papers hereh-index 6101 citations15 works total

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

author position
  • first author1
  • middle author2
  • last author1

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

fields
  • astro-ph.GA4
same name
  • Yue Cao — 19 papers
  • Yue Cao — 19 papers, h 30
  • Yue Cao — 8 papers
  • Yue Cao — 8 papers
  • Yue Cao — 5 papers, h 17
  • Yue Cao — 5 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

activity
20182021
most citedDR 21 South Filament: a Parsec-sized Dense Gas Accretion Flow onto the DR 21 Massive Young Cluster

21 citations · 31 across the 3 of their papers we have counts for

collaborators

4 papers

astro-ph.GA2021★ 10 cited

The discovery of the largest gas filament in our Galaxy, or a new spiral arm?

Chong Li, Keping Qiu, Bo Hu +1

Using the Five-hundred-meter Aperture Spherical radio Telescope (FAST), we detect a giant HI filamentary structure in the sky region of 307.∘7 < α < 311$.\!\!^{\…

astro-ph.GA2021

Core mass function of a single giant molecular cloud complex with ~10^4 cores

Yue Cao, Keping Qiu, Qizhou Zhang +2

Similarity in shape between the initial mass function (IMF) and the core mass functions (CMFs) in star-forming regions prompts the idea that the IMF originates from the CMF through…

astro-ph.GA2020★ 21 cited

DR 21 South Filament: a Parsec-sized Dense Gas Accretion Flow onto the DR 21 Massive Young Cluster

Bo Hu, Keping Qiu, Yue Cao +8

DR21 south filament (DR21SF) is a unique component of the giant network of filamentary molecular clouds in the north region of Cygnus X complex. Unlike the highly fragmented and st…

astro-ph.GA2018

An Isothermal Outflow in High-mass Star-forming Region G240.31+0.07

Junhao Liu, Keping Qiu, Friedrich Wyrowski +4

We present Atacama Pathfinder EXperiment (APEX) observations toward the massive star-forming region G240.31+0.07 in the CO J = 3--2, 6--5, and 7--6 lines. We detect a parsec-sized,…

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