activity
20142024
most citedSpectral Modeling of the Charge-Exchange X-ray Emission from M82

45 citations · 103 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.HE2024

A Monte-Carlo Simulation on Resonant Scattering of X-ray Line Emission in Supernova Remnants

Yiping Li, Gao-Yuan Zhang, Yang Chen +2

Resonant scattering (RS) of X-ray line emission in supernova remnants (SNRs) may modify the observed line profiles and fluxes and has potential impact on estimating the physical pr…

astro-ph.GA202319 cited

Scientific Objectives of the Hot Universe Baryon Surveyor (HUBS) Mission

Joel Bregman, Renyue Cen, Yang Chen +51

The Hot Universe Baryon Surveyor (HUBS) is a proposed space-based X-ray telescope for detecting X-ray emissions from the hot gas content in our universe. With its unprecedented spa…

astro-ph.SR20227 cited

Hierarchical Structure of YSO Clusters in the W40 and Serpens South Region: Group Extraction and Comparison with Fractal Clusters

Jia Sun, Robert A. Gutermuth, Hongchi Wang +2

Young stellar clusters are believed to inherit the spatial distribution like hierarchical structures of their natal molecular cloud during their formation. However, the change of t…

astro-ph.SR202211 cited

Deep Near-Infrared Survey Toward the W40 and Serpens South Region in Aquila Rift: A Comprehensive Catalog of Young Stellar Objects

Jia Sun, Robert A. Gutermuth, Hongchi Wang +5

Active star forming regions are excellent laboratories for studying the origins and evolution of young stellar object (YSO) clustering. The W40 - Serpens South region is such a reg…

astro-ph.HE201616 cited

Evolution of High-Energy Particle Distribution in Mature Shell-Type Supernova Remnants

Houdun Zeng, Yuliang Xin, Siming Liu +3

Multi-wavelength observations of mature supernova remnants (SNRs), especially with recent advances in gamma-ray astronomy, make it possible to constrain energy distribution of ener…

astro-ph.GA20145 cited

Modeling Warm Absorption in HST/COS Spectrum of Mrk 290 with XSTAR

S. N. Zhang, L. Ji, T. R. Kallman +4

We present a new method to model a HST/COS spectrum, aimed to analyze intrinsic UV absorption from the outflow of Mrk 290, a Seyfert I galaxy. We use newly updated XSTAR to generat…