activity
20052023
most citedEvolution of rapidly rotating metal-poor massive stars towards gamma-ray bursts

601 citations · 3.2k across the 53 of their papers we have counts for

collaborators

53 papers

astro-ph.HE2023★ 4 cited

Near-Infrared Spectroscopy of Dense Ejecta Knots in the Outer Eastern Area of the Cassiopeia A Supernova Remnant

Bon-Chul Koo, Yong-Hyun Lee, Jae-Joon Lee +1

The Cassiopeia A supernova remnant has a complex structure, manifesting the multidimensional nature of core-collapse supernova explosions. To further understand this, we carried ou…

astro-ph.SR2023★ 9 cited

He abundance of Dense Circumstellar Clumps in the Cassiopeia A Supernova Remnant

Bon-Chul Koo, Dongkok Kim, Sung-Chul Yoon +1

We report on the result of He abundance analysis of dense circumstellar clumps in the young supernova remnant Cassiopeia A. These clumps, which are called quasi-stationary flocculi…

astro-ph.HE2022★ 8 cited

Near-Infrared and Optical Observations of Type Ic SN 2021krf: Luminous Late-time Emission and Dust Formation

Aravind P. Ravi, Jeonghee Rho, Sangwook Park +29

We present near-infrared (NIR) and optical observations of the Type Ic supernova (SN Ic) SN 2021krf obtained between days 13 and 259 at several ground-based telescopes. The NIR spe…

astro-ph.GA2022★ 8 cited

Red supergiant stars in IC 1613 and metallicity-dependent mixing length in the evolutionary model

Sang-Hyun Chun, Sung-Chul Yoon, Heeyoung Oh +2

We report a spectroscopic study on red supergiant stars (RSGs) in the irregular dwarf galaxy IC 1613 in the Local Group. We derive the effective temperatures () and…

astro-ph.SR2022★ 4 cited

Mass loss of massive helium star supernova progenitors shortly before explosion constrained by supernova radio properties

Takashi J. Moriya, Sung-Chul Yoon

Mass loss of massive helium stars is not well understood even though it plays an essential role in determining their remnant neutron-star or black-hole masses as well as ejecta mas…

astro-ph.SR2022★ 37 cited

Stripped-envelope stars in different metallicity environments. II. Type I supernovae and compact remnants

David R. Aguilera-Dena, Bernhard Müller, John Antoniadis +4

Stripped-envelope stars can be observed as Wolf-Rayet (WR) stars, or as less luminous hydrogen-poor stars with low mass loss rates and transparent winds. Both types are potential p…