activity
20242026
collaborators

5 papers

astro-ph.GA2026

The Extinction Distance of Supernova Remnants in Combination with the CO Line Measurements

Zhe Zhang, Jun Li, Biwei Jiang +2

Accurate distance measurements to supernova remnants (SNRs) are crucial for understanding their physical properties and evolution. We present a novel method that combines CO line o…

astro-ph.EP2025

The Detectability of Lunar-Origin Asteroids in the LSST Era

Yixuan Wu, Yifei Jiao, Wen-Yue Dai +5

While most near-Earth asteroids (NEAs) are thought to originate from the main belt, recent discoveries have suggested the existence of a lunar-derived NEA population, such as the a…

astro-ph.GA2025

Observational Evidence of Dust Evolution in Supernova Remnants: Size Redistribution Toward Larger Grains in Early Sedov Phase

He Zhao, Bingqiu Chen, Jun Li

Recent observations have revealed that dust is widespread and abundant in galaxies up to , significantly influencing their appearance and spectral properties. I…

astro-ph.GA2025

Exploring the Wolf Approach to Constraining NIR Extinction Laws in the Corona Australis Molecular Cloud

Botao Jiang, Jun Li, Xi Chen

The viability of the star count (Wolf) method is assessed as a means of constraining the near-infrared (NIR) extinction law toward the Corona Australis molecular cloud. Using deep…

astro-ph.GA2024

The Flattest Infrared Extinction Curve in Four Isolated Dense Molecular Cloud Cores

Jun Li, Bingqiu Chen, Biwei Jiang +3

The extinction curve of interstellar dust in the dense molecular cloud cores is crucial for understanding dust properties, particularly size distribution and composition. We invest…