activity
20052023
most citedLocking of the Rotation of Disk-Accreting Magnetized Stars

182 citations · 615 across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.HE2023★ 2 cited

The X-ray variation of M81* resolved by Chandra and NuSTAR

S. Niu, F. G. Xie, Q. D. Wang +3

Despite advances in our understanding of low luminosity active galactic nuclei (LLAGNs), the fundamental details about the mechanisms of radiation and flare/outburst in hot accreti…

astro-ph.SR2022★ 7 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.SR2022★ 11 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.GA2022★ 4 cited

X-ray Spectroscopic Evidence of Charge Exchange Emission in the Disk of M51

Shuinai Zhang, Q. Daniel Wang, Wei Sun +3

In the disks of spiral galaxies, diffuse soft X-ray emission is known to be strongly correlated with star-forming regions. However, this emission is not simply from a thermal-equil…

astro-ph.HE2013★ 46 cited

Three-dimensional Simulations of Pure Deflagration Models for Thermonuclear Supernovae

Min Long, George C. Jordan, Daniel R. van Rossum +6

We present a systematic study of the pure deflagration model of Type Ia supernovae using three-dimensional, high-resolution, full-star hydrodynamical simulations, nucleosynthetic y…

astro-ph.CO2013★ 5 cited

Comparing the light curves of simulated Type Ia Supernovae with observations using data-driven models

Benedikt Diemer, Richard Kessler, Carlo Graziani +4

We propose a robust, quantitative method to compare the synthetic light curves of a Type Ia Supernova (SNIa) explosion model with a large set of observed SNeIa, and derive a figure…