activity
20152026
most citedRadiative Transfer in Lyα Nebulae: I. Modeling a Continuous or Clumpy Spherical Halo with a Central Source

19 citations · 89 across the 13 of their papers we have counts for

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Showing astro-ph.SRShow all

9 papers · 1 filter

astro-ph.SR2026

High-Resolution Spectroscopy of Raman-scattered He II Lines in the Symbiotic Nova RR Telescopii

Jaejin Shin, Seok-Jun Chang, Hee-Won Lee +1

Raman-scattered emission features in symbiotic stars provide a powerful diagnostic of mass-loss and transfer processes, as they uniquely probe both ionized and neutral regions with…

astro-ph.SR2025

High Resolution {\it BOES} Spectroscopy of Raman-scattered He~II6545 in Young Planetary Nebulae

Jin Lim, Seok-Jun Chang, Jaejin Shin +5

Young planetary nebulae (PNe) are characterized by their hot central stars and the presence of abundant neutral and molecular components, which result from significant mass loss du…

astro-ph.SR2023★ 1 cited

Twenty-Five Years of Accretion onto the Classical T Tauri Star TW Hya

Gregory J. Herczeg, Yuguang Chen, Jean-Francois Donati +39

Accretion plays a central role in the physics that governs the evolution and dispersal of protoplanetary disks. The primary goal of this paper is to analyze the stability over time…

astro-ph.SR2023★ 2 cited

Distribution and Kinematics of H I through Raman He II Spectroscopy of NGC 6302

Seok-Jun Chang, Hee-Won Lee, Jiyu Kim +1

The young planetary nebula NGC 6302 is known to exhibit Raman-scattered He II features at 6545 and 4851 Angstrom. These features are formed through inelastic scattering of He II$λλ…

astro-ph.SR2023★ 10 cited

Lyman-alpha Scattering Models Trace Accretion and Outflow Kinematics in T Tauri Systems

Nicole Arulanantham, Max Gronke, Eleonora Fiorellino +18

T Tauri stars produce broad Lyman-alpha emission lines that contribute 88% of the total UV flux incident on the inner circumstellar disks. Lyman-alpha photons are generated a…

astro-ph.SR2020

3D Grid-Based Monte Carlo Code for Radiative Transfer through Raman and Rayleigh Scattering with Atomic Hydrogen -- STaRS

Seok-Jun Chang, Hee-Won Lee

Emission features formed through Raman scattering with atomic hydrogen provide unique and crucial information to probe the distribution and kinematics of a thick neutral region ill…

astro-ph.SR2019★ 5 cited

Line Formation of Raman-Scattered He II 4851 in an Expanding Spherical H I Shell in Young Planetary Nebulae

Bo-Eun Choi, Seok-Jun Chang, Ho-Gyu Lee +1

We investigate line formation of Raman-scattered He II at 4851 in an expanding neutral spherical shell that surrounds a point-like He II source located at the center. A new grid-ba…

astro-ph.SR2018★ 8 cited

Broad Wings around H and H in the Two S-Type Symbiotic Stars Z Andromedae and AG Draconis

Seok-Jun Chang, Hee-Won Lee, Ho-Gyu Lee +3

Symbiotic stars often exhibit broad wings around Balmer emission lines, whose origin is still controversial. We present the high resolution spectra of the S type symbiotic stars Z…

astro-ph.SR2016★ 4 cited

A Monte Carlo Study of Flux Ratios of Raman Scattered O~VI Features at 6825 Å and 7082 Å in Symbiotic Stars

Young-Min Lee, Dae-Sub Lee, Seok-Jun Chang +2

Symbiotic stars are regarded as wide binary systems consisting of a hot white dwarf and a mass losing giant. They exhibit unique spectral features at 6825 Å and 7082 Å, which are f…