0000000001270580

AUTHOR

Marco Limongi

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

2021

LBVs are massive evolved stars that suffer sporadic and violent mass-loss events. They have been proposed as the progenitors of some core-collapse SNe, but this idea is still debated due to the lack of direct evidence. Since SNRs can carry in their morphology the fingerprints of the progenitor stars as well as of the inhomogeneous CSM sculpted by the progenitors, the study of SNRs from LBVs could help to place core-collapse SNe in context with the evolution of massive stars. We investigate the physical, chemical and morphological properties of the remnants of SNe originating from LBVs, in order to search for signatures, revealing the nature of the progenitors, in the ejecta distribution and…

Shock waveAstrophysics::High Energy Astrophysical Phenomenamedia_common.quotation_subjectStrong interactionSupernovae: generalFOS: Physical sciencesContext (language use)Astrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsAsymmetryStars: individual: Gal 026.47+0.02Settore FIS/05 - Astronomia E AstrofisicaAstrophysics::Solar and Stellar AstrophysicsStars: massiveEjectaAstrophysics::Galaxy AstrophysicsSolar and Stellar Astrophysics (astro-ph.SR)ISM: supernova remnantsmedia_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsAstronomy and AstrophysicsSupernovaStarsAstrophysics - Solar and Stellar AstrophysicsLuminous blue variableSpace and Planetary ScienceHydrodynamicsAstrophysics - High Energy Astrophysical PhenomenaAstronomy & Astrophysics
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