collaborators

5 papers

astro-ph.HE2026

Chandra and XMM-Newton X-ray Study on the Core-collapse Supernova Remnant N63A in an H II Region

Hanxiao Chen, Yang Chen, Lei Sun +1

N63A is one of the brightest supernova remnants (SNRs) in the Large Magellanic Cloud and provides an excellent laboratory for studying SNR evolution in an H II region. We present a…

astro-ph.HE2026

A pulsar escaping an ancient open cluster via tidal stripping

Lei Zhang, Xiaoting Fu, Di Li +21

Open clusters are the primary birthplaces of stars in the Milky Way disk, yet their neutron star progeny are rarely found within them, presumably due to supernova-induced kicks tha…

astro-ph.SR2026

Review of Machine Learning Models for Solar Energetic Particle Prediction

Spiridon Kasapis, Pouya Hosseinzadeh, Kathryn Whitman +73

Solar energetic particle (SEP) events have attracted increasing attention due to their significant radiation hazards for aviation, spacecraft electronics, and human missions beyond…

astro-ph.HE2025

Evolution of X-ray Gas in SN 1987A from 2007 to 2021: Ring Fading and Ejecta Brightening Unveiled through Differential Emission Measure Analysis

Lei Sun, Salvatore Orlando, Emanuele Greco +4

As the nearest supernova (SN) observed since Kepler's SN of 1604, SN 1987A provides an unprecedented opportunity to study in detail the early evolution of supernova remnants (SNRs)…

astro-ph.HE2025

Unusual X-ray Oxygen Line Ratios of SN 1987A Arising From the Absorption of Galactic Hot Interstellar Medium

Lei Sun, Salvatore Orlando, Emanuele Greco +5

Recent high-resolution X-ray spectroscopic studies have revealed unusual oxygen line ratios, such as the high O VII forbidden-to-resonance ratio, in several supernova remnants. Whi…