Results 61 to 70 of about 405 (141)
CSI in Supernova Remnants [PDF]
, 2017 Supernovae (SNe) explode in environments that have been significantly modified by the SN progenitors. For core-collapse SNe, the massive progenitors ionize the ambient interstellar medium (ISM) via UV radiation and sweep the ambient ISM via fast stellar ...
You-Hua Chu
core +1 more source
Structure distribution and turbulence in self-consistently supernova-driven ISM of multiphase magnetized galactic discs [PDF]
, 2017 International audienceContext. Galaxy evolution and star formation are two multi-scale problems tightly linked to each other.Aims. We aim to describe simultaneously the large-scale evolution widely induced by the feedback processes and the details of the
Olivier Iffrig +3 more
core +1 more source
The supernova remnant SN 1006 as a Galactic particle accelerator. [PDF]
Nat Commun, 2022 Giuffrida R +8 more
europepmc +1 more source
Continuous solutions of cosmic-rays and waves in astrophysical environments. [PDF]
Sci Rep, 2023 Irshad K +5 more
europepmc +1 more source
87th Annual Meeting of the Meteoritical Society 2025: Abstracts
Meteoritics &Planetary Science, Volume 60, Issue S1, Page 30-350, August 2025.
wiley +1 more source
Revealing a peculiar supernova remnant G106.3+2.7 as a petaelectronvolt proton accelerator with X-ray observations. [PDF]
Innovation (Camb), 2021 Ge C, Liu RY, Niu S, Chen Y, Wang XY.
europepmc +1 more source
The relativistic ISM in M33: Role of the supernova remnants
The Astrophysical Journal, 1995 N. Duric +4 more
openaire +1 more source
86th Annual Meeting of the Meteoritical Society (2024)
Meteoritics &Planetary Science, Volume 59, Issue S1, Page A1-A468, August 2024.
wiley +1 more source