activity
20242026
collaborators

6 papers

astro-ph.HE2026

Unraveling the mysteries of supernovae with SKA+VLBI

Tao An, Zhengwei Liu, Ailing Wang +6

Supernovae (SNe) drive cosmic chemical enrichment and shape galactic feedback, yet the link between progenitors and explosion outcomes remains poorly constrained because the earlie…

astro-ph.SR2026

The outer rings of SN 1987A from year 1994 to 2024: morphology, light curves, and optical to mid-infrared spectra

Sophie Rosu, Elko Gerville-Reache, Steven Thomas +14

The outer rings (ORs) of Supernova (SN) 1987A were ejected ~20000 years before the explosion. Their characterisation is crucial for constraining the properties of the progenitor of…

astro-ph.HE2026

Exploring the central region of SNR 0540-69.3 with JWST I: 3D morphology

J. Larsson, C. Tegkelidis, C. Fransson +3

The young supernova remnant SNR 0540-69.3 in the Large Magellanic Cloud offers a detailed view of an energetic pulsar-wind nebula interacting with the surrounding ejecta. We presen…

astro-ph.HE2025

MUSE Observations Reveal Optical Coronal Iron Lines from Shock Emission in Supernova Remnant 0540-69.3

L. Tenhu, J. Larsson, P. Lundqvist +3

We investigate the optical shock emission from the Large Magellanic Cloud supernova remnant 0540-69.3 (SNR 0540) using MUSE integral-field-unit data from the VLT. The observations…

astro-ph.HE2025

Teleios (G305.4-2.2) -- the mystery of a perfectly shaped new Galactic supernova remnant

Miroslav D. Filipovic, Zachary J. Smeaton, Roland Kothes +35

We present the serendipitous radio-continuum discovery of a likely Galactic supernova remnant (SNR) G305.4-2.2. This object displays a remarkable circular symmetry in shape, making…

astro-ph.HE2024

The radial distribution of radio emission from SN1993J: Magnetic field amplification due to the Rayleigh-Taylor instability

I. Marti-Vidal, C-I. Bjornsson, M. A. Perez-Torres +2

[SHORTENED VERSION] Observations of radio emission from young core-collapse supernovae (CCSNe) allow one to study the history of the pre-supernova stellar wind, trace the density s…