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Simulations of the W50-SS433 system

Published online by Cambridge University Press:  07 April 2020

Dimitrios Millas Open the ORCID record for Dimitrios Millas [Opens in a new window] ,
Oliver Porth  and
Rony Keppens
Dimitrios Millas
Affiliation:
Centre for mathematical Plasma Astrophysics, KU Leuven, Celestijnenlaan 200B, 3001, Leuven, Belgium email: dimitrios.millas@kuleuven.be
Oliver Porth
Affiliation:
Institut für Theoretische Physik, Goethe-Universität Frankfurt am Main, Max-von-Laue-Str. 1, 60438, Frankfurt am Main, Germany
Rony Keppens
Affiliation:
Centre for mathematical Plasma Astrophysics, KU Leuven, Celestijnenlaan 200B, 3001, Leuven, Belgium email: dimitrios.millas@kuleuven.be
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Abstract

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Supernovae and astrophysical jets are two of the most energetic and intriguing objects in the universe. We examine an interesting scenario that involves the interaction of these two extreme phenomena, motivated by observations of the W50-SS433 system: a jet launched from the microquasar SS433 (an X-ray binary) located inside a supernova remnant, W50. These observations revealed a unique morphology of the remnant, attributed to the presence of the jet. We performed full 3D relativistic hydrodynamic simulations to better capture the interaction between the remnant and the jet and post-processed the data with a radiative transfer code to create emission maps.

Keywords

hydrodynamicsmethods: numerical(stars:) supernovae: generalISM: jets and outflows(ISM:) supernova remnants
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium S342: Perseus in Sicily: From Black Hole to Cluster Outskirts , May 2018 , pp. 257 - 259
Copyright
© International Astronomical Union 2020

References

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