activity
20162026
most citedA high resolution HI study towards the supernova remnant Puppis A and its environments

44 citations · 66 across the 6 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

5 papers · 1 filter

astro-ph.HE2026

Molecular and Atomic Gas Associated with the Gamma Ray Supernova Remnant RCW 103

H. Inoue, Y. Asano, R. G. Bhuvana +15

We present a study of the interstellar molecular and atomic gas associated with the gamma-ray supernova remnant (SNR) RCW 103 using the Mopra CO( = 1-0), Atacama Large Mi…

astro-ph.HE2025★ 3 cited

X-ray polarization in SN 1006 southwest shows spatial variations and differences with the radio band

Ping Zhou, Patrick Slane, Dmitry Prokhorov +15

We report the detection of a spatial variation of X-ray polarization in the southwestern shell of SN 1006 (SN 1006 SW) using IXPE. The shell has an average X-ray polarization degre…

astro-ph.HE2023

Magnetic structures and turbulence in SN 1006 revealed with imaging X-ray polarimetry

Ping Zhou, Dmitry Prokhorov, Riccardo Ferrazzoli +99

Young supernova remnants (SNRs) strongly modify surrounding magnetic fields, which in turn play an essential role in accelerating cosmic rays (CRs). X-ray polarization measurements…

astro-ph.HE2018

Possible Evidence for Cosmic-Ray Acceleration in the Type Ia SNR RCW 86: Spatial Correlation between TeV Gamma rays and Interstellar Atomic Protons

H. Sano, G. Rowell, E. M. Reynoso +13

We present a detailed morphological study of TeV gamma rays, synchrotron radiation, and interstellar gas in the young Type Ia supernova remnant (SNR) RCW 86. We find that the inter…

astro-ph.HE2017★ 15 cited

A 3D MHD simulation of SN 1006: a polarized emission study for the turbulent case

P. F. Velázquez, E. M. Schneiter, E. M. Reynoso +6

Three dimensional magnetohydrodynamical simulations were carried out in order to perform a new polarization study of the radio emission of the supernova remnant SN 1006. These simu…