Observational signatures of particle acceleration in supernova remnants

EA Helder, J Vink, AM Bykov, Y Ohira… - Space Science …, 2012 - Springer
We evaluate the current status of supernova remnants as the sources of Galactic cosmic
rays. We summarize observations of supernova remnants, covering the whole …

Storage ring at HIE-ISOLDE: Technical design report

M Grieser, YA Litvinov, R Raabe, K Blaum… - The European Physical …, 2012 - Springer
We propose to install a storage ring at an ISOL-type radioactive beam facility for the first
time. Specifically, we intend to setup the heavy-ion, low-energy ring TSR at the HIE-ISOLDE …

Production of 44Ti and Iron-group Nuclei in the Ejecta of 3D Neutrino-driven Supernovae

A Sieverding, D Kresse, HT Janka - The Astrophysical Journal …, 2023 - iopscience.iop.org
The radioactive isotopes 44 Ti and 56 Ni are important products of explosive
nucleosynthesis, which play a key role in supernova (SN) diagnostics and have been …

Production and distribution of 44Ti and 56Ni in a three-dimensional supernova model resembling Cassiopeia A

A Wongwathanarat, HT Janka, E Müller… - The Astrophysical …, 2017 - iopscience.iop.org
The spatial and velocity distributions of nuclear species synthesized in the innermost
regions of core-collapse supernovae can yield important clues about explosion asymmetries …

The expansion asymmetry and age of the Cassiopeia A supernova remnant

RA Fesen, MC Hammell, J Morse… - The Astrophysical …, 2006 - iopscience.iop.org
HST images of the young supernova remnant Cas A are used to explore the expansion and
spatial distribution of its highest velocity debris. ACS WFC images taken in 2004 March and …

X-ray polarization detection of Cassiopeia A with IXPE

J Vink, D Prokhorov, R Ferrazzoli, P Slane… - The Astrophysical …, 2022 - iopscience.iop.org
We report on a∼ 5σ detection of polarized 3–6 keV X-ray emission from the supernova
remnant Cassiopeia A (Cas A) with the Imaging X-ray Polarimetry Explorer (IXPE). The …

The dynamics, destruction, and survival of supernova-formed dust grains

JD Slavin, E Dwek, MM Mac Low… - The Astrophysical …, 2020 - iopscience.iop.org
Observations have demonstrated that supernovae efficiently produce dust. This is consistent
with the hypothesis that supernovae and asymptotic giant branch stars are the primary …

The dust mass in Cassiopeia A from a spatially resolved Herschel analysis

I De Looze, MJ Barlow, BM Swinyard… - Monthly Notices of …, 2016 - academic.oup.com
Theoretical models predict that core-collapse supernovae (CCSNe) can be efficient dust
producers (0.1-1.0 M⊙), potentially accounting for most of the dust production in the early …

[BOOK][B] Physics and evolution of supernova remnants

J Vink - 2020 - Springer
When I started working on my PhD project on X-ray spectroscopy of supernova remnants in
1995, one of the things that I missed was a good textbook covering the various aspects of …

The fully developed remnant of a neutrino-driven supernova-Evolution of ejecta structure and asymmetries in SNR Cassiopeia A

S Orlando, A Wongwathanarat, HT Janka… - Astronomy & …, 2021 - aanda.org
Context. The remnants of core-collapse supernovae (SNe) are probes of the physical
processes associated with their parent SNe. Aims. Here we aim to explore to which extent …