activity
20132023
most citedThermal radio absorption as a tracer of the interaction of SNRs with their environments

22 citations · 77 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.GA2023

One size fits all: Insights on Extrinsic Thermal Absorption from Similarity of Supernova Remnant Radio Continuum Spectra

M. G. Abadi, G. Castelletti, L. Supan +2

Typically, integrated radio frequency continuum spectra of supernova remnants (SNRs) exhibit a power-law form due to their synchrotron emission. In numerous cases, these spectra sh…

astro-ph.HE2022★ 7 cited

Supernova remnant G46.8-0.3, a new case of interaction with molecular material

L. Supan, G. Fischetto, G. Castelletti

We present the first detailed study on the Galactic supernova remnant (SNR) G46.8-0.3 and its environment since its discovery more than 50 years ago. With new flux measurements fro…

astro-ph.HE2021★ 22 cited

Thermal radio absorption as a tracer of the interaction of SNRs with their environments

G. Castelletti, L. Supan, W. M. Peters +1

We present new images and continuum spectral analysis for 14 resolved Galactic SNRs selected from the 74 MHz Very Large Array Low-Frequency Sky Survey Redux (VLSSr). We combine new…

astro-ph.HE2019

New X-ray observations toward PSR J1826-1256

L. Duvidovich, E. Giacani, G. Castelletti +2

We present the results of XMM-Newton observations toward the pulsar PSR J18261256, which lies at 5.4 from the centroid of the TeV source HESS J1826130. These data…

astro-ph.HE2018★ 1 cited

A revisited study of the unidentified -ray emission towards the SNR Kes 41

Leonardo Supan, Gabriela Castelletti, Alberto D. Supanitsky +1

Kes 41 is among the Galactic supernova remnants (SNRs) proposed to be physically linked to -ray emission at GeV energies. Although not conclusively, the nature of the -ray ph…

astro-ph.HE2018★ 2 cited

Natal molecular cloud of SNR Kes 41. Complete characterisation

Leonardo Supán, Gabriela Castelletti, Alberto D. Supanitsky +3

Using high-resolution data of the CO and CO (=1-0}) line emission from The Mopra Southern Galactic Plane CO Survey in conjunction with neutral hydrogen observation…