activity
20122026
most citedThe ice composition in the disk around V883 Ori revealed by its stellar outburst

140 citations · 399 across the 23 of their papers we have counts for

collaborators

23 papers

astro-ph.EP2026★ 7 cited

Accretion Burst Crystallizes Silicates in a Planet-Forming Disk

Jeong-Eun Lee, Chul-Hwan Kim, Jaeyeong Kim +13

Crystalline silicates form at high temperatures (> 900 K; Fabian et al. 2000; Hallenbeck et al. 1998). Their presence in comets (Hanner et al. 1994; Hayward et al. 2000; Wooden et…

astro-ph.GA2026

EPISODE II: Variability in the CO and HO rovibrational absorption lines in a periodically variable protostar EC 53

Seokho Lee, Jeong-Eun Lee, Chul-Hwan Kim +19

We present two-epoch JWST NIRSpec and MIRI observations of the young protostar EC 53 (V371 Ser), a periodically variable source with well-characterized quiescent and burst phases.…

astro-ph.SR2026

EPISODE IV: Ice Inventory in the Envelope of EC 53

Jaeyeong Kim, Jeong-Eun Lee, Chul-Hwan Kim +9

We present the 1.628 m spectra of the young protostar EC 53, obtained with JWST NIRSpec IFU and MIRI MRS during the quiescent and burst phases of its periodic brightness vari…

astro-ph.SR2025★ 1 cited

Water Snowline in Young Stellar Objects with Various Density Structures Using Radiative Transfer Models

Young-Jun Kim, Jeong-Eun Lee, Giseon Baek +1

Tracing the water snowline in low-mass young stellar objects (YSOs) is important because dust grain growth is promoted and the chemical composition varies at the water snowline, wh…

astro-ph.GA2025

The robust detection and spatial distribution of acetaldehyde in Orion KL: ALMA observations and chemical modeling

Miwha Jin, Anthony J. Remijan, Robin T. Garrod +5

Despite the organic molecule inventory detected in Orion KL, acetaldehyde (CH3CHO) -- one of the most ubiquitous interstellar aldehydes -- has not been firmly identified with mm-wa…

astro-ph.SR2024

ALMA Spectral Survey of An eruptive Young star, V883 Ori (ASSAY): II. Freshly Sublimated Complex Organic Molecules (COMs) in the Keplerian Disk

Jae-Hong Jeong, Jeong-Eun Lee, Seonjae Lee +9

We present an investigation of Complex Organic Molecules (COMs) in the spatially resolved Keplerian disk around V883 Ori, an eruptive young star, based on a spectral survey carried…

astro-ph.SR2024

A Natural Laboratory for Astrochemistry, a Variable Protostar B335

Jeong-Eun Lee, Neal J. Evans, Giseon Baek +3

Emission lines from complex organic molecules in B335 were observed in four epochs, spanning a luminosity burst of about 10 years duration. The emission lines increased dramaticall…

astro-ph.SR2024

ALMA Spectral Survey of An eruptive Young star, V883 Ori (ASSAY): I. What triggered the current episode of eruption?

Jeong-Eun Lee, Chul-Hwan Kim, Seokho Lee +7

An unbiased spectral survey of V883 Ori, an eruptive young star, was carried out with the Atacama Large Millimeter/submillimeter Array (ALMA) in Band 6. The detected line emission…

astro-ph.SR2023★ 5 cited

Spectral survey of a Hot core with an Eruptive Accretion in S255IR NIRS3 (SHEA): The discovery of class I and class II millimeter methanol maser transitions

Giseon Baek, Jeong-Eun Lee, Neal J. Evans +5

We report the detection of the millimeter CHOH masers including a new detection of class I (11-10A) and class II (6-5E) maser transitions towa…

astro-ph.SR2023

Complex Organic Molecules in a Very Young Hot Corino, HOPS 373SW

Jeong-Eun Lee, Giseon Baek, Seokho Lee +6

We present the spectra of Complex Organic Molecules (COMs) detected in HOPS 373SW with the Atacama Large Millimeter/submillimeter Array (ALMA). HOPS 373SW, which is a component of…

astro-ph.GA2022★ 22 cited

Complex organic molecules detected in twelve high-mass star-forming regions with Atacama Large Millimeter/submillimeter Array (ALMA)

Giseon Baek, Jeong-Eun Lee, Tomoya Hirota +2

Recent astrochemical models and experiments have explained that complex organic molecules (COMs; molecules composed of six or more atoms) are produced on the dust grain mantles in…

astro-ph.GA2021

TIMES II: Investigating the Relation Between Turbulence and Star-forming Environments in Molecular Clouds

Hyeong-Sik Yun, Jeong-Eun Lee, Neal J. Evans +14

We investigate the effect of star formation on turbulence in the Orion A and Ophiuchus clouds using principal component analysis (PCA). We measure the properties of turbulence by a…

astro-ph.SR2021★ 2 cited

The JCMT Transient Survey: Four Year Summary of Monitoring the Submillimeter Variability of Protostars

Yong-Hee Lee, Doug Johnstone, Jeong-Eun Lee +49

We present the four-year survey results of monthly submillimeter monitoring of eight nearby (pc) star-forming regions by the JCMT Transient Survey. We apply the Lomb-Scargl…

astro-ph.GA2021★ 11 cited

TIMES I: a Systematic Observation in Multiple Molecular Lines Toward the Orion A and Ophiuchus Clouds

Hyeong-Sik Yun, Jeong-Eun Lee, Yunhee Choi +16

We have used the Taeduk Radio Astronomy Observatory to observe the Orion A and Ophiuchus clouds in the 10 lines of CO, CO, HCN, HCO, and NH and the…

astro-ph.SR2020★ 37 cited

Young Faithful: The Eruptions of EC 53 as It Cycles through Filling and Draining the Inner Disk

Yong-Hee Lee, Doug Johnstone, Jeong-Eun Lee +10

While young stellar objects sometimes undergo bursts of accretion, these bursts usually occur sporadically, making them challenging to study observationally and to explain theoreti…

astro-ph.SR2020★ 41 cited

The Relationship between Mid-Infrared and Sub-Millimetre Variability of Deeply Embedded Protostars

Carlos Contreras Peña, Doug Johnstone, Giseon Baek +5

We study the relationship between the mid-infrared and sub-mm variability of deeply embedded protostars using the multi-epoch data from the Wide Infrared Survey Explorer (/NE…

astro-ph.SR2020★ 33 cited

Radiative Transfer modeling of EC 53: An Episodically Accreting Class I Young Stellar Object

Giseon Baek, Benjamin A. MacFarlane, Jeong-Eun Lee +8

In the episodic accretion scenario, a large fraction of the protostellar mass accretes during repeated and large bursts of accretion. Since outbursts on protostars are typically id…

astro-ph.SR2019★ 27 cited

Observational signatures of outbursting protostars -- II: Exploring a wide range of eruptive protostars

Benjamin MacFarlane, Dimitris Stamatellos, Doug Johnstone +5

Young stars exhibit variability due to changes in the gas accretion rate onto them, an effect that should be quite significant in the early stages of their formation. As protostars…

astro-ph.SR2019★ 25 cited

Observational signatures of outbursting protostars - I: From hydrodynamic simulations to observations

Benjamin MacFarlane, Dimitris Stamatellos, Doug Johnstone +5

Accretion onto protostars may occur in sharp bursts. Accretion bursts during the embedded phase of young protostars are probably most intense, but can only be inferred indirectly t…

astro-ph.SR2018★ 140 cited

The ice composition in the disk around V883 Ori revealed by its stellar outburst

Jeong-Eun Lee, Seokho Lee, Giseon Baek +6

Complex organic molecules (COMs), which are the seeds of prebiotic material and precursors of amino acids and sugars, form in the icy mantles of circumstellar dust grains but canno…

astro-ph.GA2017★ 13 cited

The Infrared Medium-deep Survey. III. Survey of Luminous Quasars at 4.7 z 5.4

Yiseul Jeon, Myungshin Im, Dohyeong Kim +21

We present our first results of the survey for high redshift quasars at . The search for quasars in this redshift range has been known to be challe…

astro-ph.SR2014★ 12 cited

Color Variability of HBC 722 in the Post-Outburst Phases

Giseon Baek, Soojong Pak, Joel D. Green +7

We carried out photometric observations for HBC 722 in SDSS r, i and z bands from 2011 April to 2013 May with a Camera for Quasars in Early uNiverse attached to the 2.1m Otto Struv…

astro-ph.GA2012★ 23 cited

Variability at the Edge: Optical Near/IR Rapid Cadence Monitoring of Newly Outbursting FU Orionis Object HBC 722

Joel D. Green, Paul Robertson, Giseon Baek +7

We present the detection of day-timescale periodic variability in the r-band lightcurve of newly outbursting FU Orionis-type object HBC 722, taken from > 42 nights of observation w…