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researcher

I. Han

38 papers hereh-index 20883 citations45 works total

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

author position
  • first author2
  • middle author31
  • last author1

Across the 34 of 38 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA19
  • astro-ph.EP11
  • astro-ph.SR8
same name
  • I. Han — 24 papers, h 19
  • I. Han — 1 paper, h 21
  • I. Han — 1 paper, h 3
  • I. Han — 1 paper, h 25
  • I. Han — 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
20172026
most citedEarly Planet Formation in Embedded Disks (eDisk). I. Overview of the Program and First Results

159 citations · 699 across the 33 of their papers we have counts for

collaborators
Showing 2025Show all

3 papers · 1 filter

astro-ph.SR2025

Early Planet Formation in Embedded Disks (eDisk) XXII: Keplerian disk, disk structures and jets/outflows in the Class 0 protostar IRAS 04166+2706

Nguyen Thi Phuong, Chang Won Lee, John J. Tobin +20

We present ALMA observations of the Class 0 protostar IRAS 04166+2706, obtained as part of the ALMA large program Early Planet Formation in Embedded Disks (eDisk). These observatio…

astro-ph.EP2025

Early Planet Formation in Embedded Disks (eDisk) XVII: A Compact but Structured Keplerian Disk and Large-scale Streamers Revealed in the Class I Protostellar System IRAS 04169+2702

Ilseung Han, Woojin Kwon, Yusuke Aso +22

We present high-resolution (∼0.05"; 8 au) dust continuum and molecular line observations toward the Class I protostellar system IRAS 04169+2702 in the Taurus B213 region, as p…

astro-ph.SR2025

Early Planet Formation in Embedded Disks (eDisk) XXI: Limited role of streamers in mass supply to the disk in the Class 0 protostar IRAS 16544-1604

Miyu Kido, Hsi-Wei Yen, Jinshi Sai +17

Asymmetric and narrow infalling structures, often called streamers, have been observed in several Class 0/I protostars, which is not expected in the classical star formation pictur…

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