Modeling the remnants of core-collapse supernovae from luminous blue variable stars

@article{Ustamujic2021ModelingTR,
  title={Modeling the remnants of core-collapse supernovae from luminous blue variable stars},
  author={Sabina Ustamujic and Salvatore Orlando and Marco Miceli and Fabrizio Bocchino and Marco Limongi and Alessandro Chieffi and Corrado Trigilio and G Umana and Filomena Bufano and Adriano Ingallinera and Giovanni Peres},
  journal={Astronomy \& Astrophysics},
  year={2021}
}
Context. Luminous blue variable stars (LBVs) are massive evolved stars that suffer sporadic and violent mass-loss events. They have been proposed as the progenitors of some core-collapse supernovae (SNe), but this idea is still debated because of a lack of strong evidence. As supernova remnants (SNRs) can carry in their morphology the fingerprints of the progenitor stars as well as of the inhomogeneous circumstellar medium (CSM) sculpted by the progenitors, the study of SNRs from LBVs could… 
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. Young core-collapse supernovae (YSNe) are factories of high-energy neutrinos and gamma-rays as the shock accelerated protons efficiently interact with the protons in the dense circumstellar medium.

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