Splinter Meeting SNR
Multiwavelength studies of supernova remnants and their impact on the interstellar medium
Time: Tuesday September 10, 14:00-16:30 and Thursday September 12, 14:00-15:45 CEST (UTC+2)
Room: S14
Convenor(s): Ekaterina Makarenko [1],
Masato Kobayashi [1},
Martin Mayer [2],
Manami Sasaki [2],
Polina Smirnova [1]
[1] 1. Institute of Physics, University of Cologne,
[2] Dr.-Remeis-Sternwarte Bamberg, Friedrich-Alexander-Universität Erlangen-Nürnberg
Supernova remnants (SNRs) play a crucial role in controlling the thermal, dynamical, magnetic, and chemical properties of galaxies and are sites of a plethora of astrophysical processes. Nowadays, we have access to large multiwavelength datasets through multiple ongoing observations of SNRs across the entire electromagnetic wavelengths range (ASKAP, MeerKAT, ALMA, Herschel, JWST, Hubble, Chandra, XRISM, eROSITA, H.E.S.S., etc.). Different wavelengths reveal various aspects of physical processes in SNRs: radio frequencies trace synchrotron emission of particles in the SNR's magnetic field, the submm and infrared bands reveal the production and destruction of dust, optical wavelengths help explore dense radiative regions within older SNRs, the X-ray band is crucial for studying the shock-heated gas within SNRs, whereas gamma-ray observations provide insights into the acceleration of cosmic rays by SNR shock fronts. By definition, SNRs are not isolated objects, as they are the manifestation of the interaction of a supernova with structures of the interstellar medium in which they explode, which may be influenced by stellar winds, or exhibit dense features like molecular clouds. Simulations of SNRs in complex environments help us bridge the gap between analytical theoretical models and the complexities of the real interstellar medium, in the attempt to accurately reproduce the observed radiative signature of SNRs at different wavelengths. By combining data from multiwavelength observations with insights from simulations, we can thereby constrain the physical properties of SNRs, including pre-supernova conditions (e.g., density, magnetic fields, turbulence), the nucleosynthetic products of the explosion, or the mechanism of particle acceleration. In this splinter session, we would like to bring together researchers working on simulations of SNRs with researchers working on observations across the electromagnetic spectrum, to gain an in-depth understanding of the life cycles of SNRs and their impact on the Galactic ecosystem.
Program
Tuesday September 10, 14:00-16:30 Multiwavelength studies of supernova remnants and their impact on the interstellar medium (S14)
Thursday September 12, 14:00-15:45 Multiwavelength studies of supernova remnants and their impact on the interstellar medium (S14)
Related contributions
Presenter | Title | Type |
---|---|---|
Cheryl Lau | Semi-confined supernovae within HII regions and their effect on the ISM | Contributed Talk |
Federico Zangrandi | Supernova Remnants Population in the Large Magellanic Cloud | Contributed Talk |
Günay Paylı | Investigation of supernova remnant IC 443 and G189.6+3.3 with LAMOST | Contributed Talk |
Jing Li | Discovery of ∼2200 new supernova remnants in 19 nearby star-forming galaxies with MUSE spectroscopy | Contributed Talk |
Leonard Romano | Cloud Formation by Supernova Implosion | Poster |
Leonard Romano | SISSI: Supernovae in a Shearing, Stratified Interstellar Medium | Contributed Talk |
Marie Prucker | Hydrodynamic Simulations of the Supernova Remnant PuppisA with PLUTO | Contributed Talk |