activity
20172024
most citedSource Imaging of a Moving Type-IV Solar Radio Burst and its Role in Tracking Coronal Mass Ejection From the Inner to the Outer Corona

31 citations · 132 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.GA2024

Stellar Population near NGC 2021: Procession of Star Formation in the South Rim of Supergiant Shell LMC 4

Po-Sheng Ou, Rui-Ching Chao, You-Hua Chu +2

Supergiant shells (SGSs) are the largest interstellar structures where heated and enriched gas flows into the host galaxy's halo. The SGSs in the Large Magellanic Cloud (LMC) are s…

astro-ph.GA2023

New Insights on 30 Dor B Revealed by High-Quality Multi-wavelength Observations

Wei-An Chen, Chuan-Jui Li, You-Hua Chu +4

The supernova remnant (SNR) 30 Dor B is associated with the \ion{H}{2} region ionized by the OB association LH99. The complex interstellar environment has made it difficult to stud…

astro-ph.GA2021★ 4 cited

The Shellless SNR B0532-67.5 in the Large Magellanic Cloud

Chuan-Jui Li, You-Hua Chu, Chen-Yu Chuang +1

The supernova remnant (SNR) B053267.5 in the Large Magellanic Cloud (LMC) was first diagnosed by its nonthermal radio emission and its SNR nature was confirmed by diffuse X-ray…

astro-ph.HE2021★ 14 cited

Forbidden Line Emission from Type Ia Supernova Remnants Containing Balmer-Dominated Shells

Chuan-Jui Li, You-Hua Chu, John C. Raymond +3

Balmer-dominated shells in supernova remnants (SNRs) are produced by collisionless shocks advancing into a partially neutral medium, and are most frequently associated with Type Ia…

astro-ph.HE2021★ 10 cited

SN 2018bsz: significant dust formation in a nearby superluminous supernova

T. -W. Chen, S. J. Brennan, R. Wesson +41

We investigate the thermal emission and the extinction from dust associated with the nearby (z = 0.0267) superluminous supernova (SLSN) 2018bsz. Our dataset combines daily-cadence,…

astro-ph.HE2021★ 17 cited

Discovery of Double-Ring Structure in the Supernova Remnant N103B: Evidence for Bipolar Winds from a Type Ia Supernova Progenitor

Hiroya Yamaguchi, Fabio Acero, Chuan-Jui Li +1

The geometric structure of supernova remnants (SNR) provides a clue to unveiling the pre-explosion evolution of their progenitors. Here we present an X-ray study of N103B (0509-68.…

astro-ph.GA2020★ 6 cited

Searching for Balmer-dominated Type Ia Supernova Remnants in M33

Chris Ding-Jyun Lin, You-Hua Chu, Po-Sheng Ou +1

We have searched for Balmer-dominated Type Ia SNRs in M33 by selecting thermal X-ray sources with ergs s, identifying associated H emission…

astro-ph.SR2019★ 26 cited

Search for Surviving Companions of Progenitors of Young LMC Type Ia Supernova Remnants

Chuan-Jui Li, Wolfgang E. Kerzendorf, You-Hua Chu +9

We have used two methods to search for surviving companions of Type Ia supernova progenitors in three Balmer-dominated supernova remnants (SNRs) in the Large Magellanic Cloud: 0519…

astro-ph.SR2018★ 31 cited

Source Imaging of a Moving Type-IV Solar Radio Burst and its Role in Tracking Coronal Mass Ejection From the Inner to the Outer Corona

V. Vasanth, Yao Chen, Maoshui Lv +5

Source imaging of solar radio bursts can be used to track energetic electrons and associated magnetic structures. Here we present a combined analysis of data at different wavelengt…

astro-ph.SR2017★ 24 cited

Physical Structures of the Type Ia Supernova Remnant N103B

Chuan-Jui Li, You-Hua Chu, Robert A. Gruendl +6

N103B is a Type Ia supernova remnant (SNR) projected in the outskirt of the superbubble around the rich cluster NGC 1850 in the Large Magellanic Cloud (LMC). We have obtained H…