activity
20152024
most citedNon-equilibrium ionization in mixed-morphology supernova remnants

36 citations · 87 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2024

A Yebes W band Line Survey towards an Unshocked Molecular Cloud of Supernova Remnant 3C391: Evidence of Cosmic-Ray-Induced Chemistry

Tian-Yu Tu, Prathap Rayalacheruvu, Liton Majumdar +3

Cosmic rays (CRs) have strong influences on the chemistry of dense molecular clouds (MCs). To study the detailed chemistry induced by CRs, we conducted a Yebes W band line survey t…

astro-ph.IM2021★ 7 cited

Performance of LHAASO-WCDA and Observation of Crab Nebula as a Standard Candle

LHAASO collaboration

The first Water Cherenkov detector of the LHAASO experiment (WCDA-1) has been operating since April, 2019. The first 10 months of data have been analyzed to test its performance by…

astro-ph.HE2019★ 36 cited

Non-equilibrium ionization in mixed-morphology supernova remnants

Gao-Yuan Zhang, Jonathan D. Slavin, Adam Foster +4

The mixed morphology class of supernova remnants (MMSNRs) comprises a substantial fraction of observed remnants and yet there is as yet no consensus on their origin. A clue to thei…

astro-ph.HE2018★ 15 cited

G7.7-3.7: a young supernova remnant probably associated with the guest star in 386 CE (SN 386)

Ping Zhou, Jacco Vink, Geng Li +1

Although the Galactic supernova rate is about 2 per century, only few supernova remnants are associated with historical records. There are a few ancient Chinese records of "guest s…

astro-ph.HE2015★ 29 cited

The Metal-enriched Thermal Composite Supernova Remnant Kesteven 41 (G337.8-0.1) in a Molecular Environment

Gao-Yuan Zhang, Yang Chen, Yang Su +3

The physical nature of thermal composite supernova remnants (SNRs) remains controversial. We have revisited the archival XMM-Newton and Chandra data of the thermal composite SNR Ke…