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Jun-Hui Zhao

42 papers hereh-index 282.4k citations85 works total

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

author position
  • first author12
  • middle author22
  • last author5

Across the 39 of 42 papers where every author was matched, so the position is known.

fields
  • astro-ph18
  • astro-ph.GA12
  • astro-ph.SR7
  • astro-ph.HE4
  • astro-ph.CO1
same name
  • Jun-Hui Zhao — 3 papers, h 1
  • Jun-Hui Zhao — 2 papers, h 4

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
19982022
most citedAn X-ray, IR, and Submillimeter Flare of Sagittarius A*

218 citations · 2.1k across the 42 of their papers we have counts for

collaborators
Showing 2010Show all

4 papers · 1 filter

astro-ph.GA2010★ 58 cited

The High-Density Ionized Gas in the Central Parsec of the Galaxy

Jun-Hui Zhao, Ray Blundell, James M. Moran +3

We report a study of the H30α line emission at 1.3 mm from the region around Sgr A* made with the Submillimeter Array at a resolution of 2\arcsec\ over a field of 60\arcsec\ (2 p…

astro-ph.SR2010★ 25 cited

A bipolar outflow from the massive protostellar core W51e2-E

Hui Shi, Jun-Hui Zhao, Jinlin Han

We present high resolution images of the bipolar outflow from W51e2, which are produced from the Submillimeter Array archival data observed for CO(3-2) and HCN(4-3) lines with angu…

astro-ph.GA2010

The High-Density Ionized Gas in the Central Parsecs of the Galaxy

Jun-Hui Zhao, Ray Blundell, James M. Moran +3

We report the results from observations of H30α line emission in Sgr A West with the Submillimeter Array at a resolution of 2\arcsec and a field of view of about 40\arcsec. The H…

astro-ph.SR2010★ 36 cited

Nature of W51e2: Massive Cores at Different Phases of Star Formation

Hui Shi, Jun-Hui Zhao, J. L. Han

We present high-resolution continuum images of the W51e2 complex processed from archival data of the Submillimeter Array (SMA) at 0.85 and 1.3 mm and the Very Large Array (VLA) at…

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