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researcher

Ho-Gyu Lee

67 papers hereh-index 212.3k citations130 works total

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

author position
  • sole author1
  • first author4
  • middle author49
  • last author4

Across the 58 of 67 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR21
  • astro-ph.GA19
  • astro-ph11
  • astro-ph.HE7
  • astro-ph.IM6
  • astro-ph.CO2
same name
  • Ho-Gyu Lee — 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

activity
19982026
most citedDynamical evolution of rotating stellar systems - II. Post-collapse, equal mass system

71 citations · 1k across the 64 of their papers we have counts for

collaborators
Showing 2013Show all

3 papers · 1 filter

astro-ph.SR2013★ 10 cited

[Fe II] 1.64 um Features of Jets and Outflows from Young Stellar Objects in the Carina Nebula

Jong-Ho Shinn, Tae-Soo Pyo, Jae-Joon Lee +11

We present [Fe II] 1.64 μm imaging observations for jets and outflows from young stellar objects (YSOs) over the northern part (~ 24'x45') of the Carina Nebula, a massive star form…

astro-ph.GA2013★ 10 cited

Wide Integral-Field Infrared Spectroscopy of the Bright [Fe II] Shell in the Young Supernova Remnant G11.2-0.3

Ho-Gyu Lee, Dae-Sik Moon, Bon-Chul Koo +9

We present the results of wide integral-field near-infrared (1.0-1.8 um) spectroscopic observations of the southeastern shell of the young core-collapse supernova remnant (SNR) G11…

astro-ph.GA2013★ 18 cited

Large-area [Fe II] Line Mapping of the Supernova Remnant IC443 with the IRSF/SIRIUS

Takuma Kokusho, Takahiro Nagayama, Hidehiro Kaneda +3

We present the result of near-infrared (near-IR) [Fe II] line mapping of the supernova remnant IC443 with the IRSF/SIRIUS, using the two narrow-band filters tuned for the [Fe II] 1…

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