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ǂThe ǂtransitional type Ibn/Iin sn 2022pda, with pre-explosion outbursts and a double-peaked light curve
Y.-Z. Cai, A. B. Newman, A. Pastorello, R. Chiba, T. J. Moriya, A. Reguitti, L. Tartaglia, S. Moran, S. Campana, T. Petrushevska
Izvirni znanstveni članek
Oznake: supernovae;core-collapse supernovae;circumstellar matter;stellar mass loss;
We report the results of a photometric and spectroscopic follow-up campaign of the unusual interacting supernova (SN) 2022pda. Precursor variability lasting ∼100 days is observed before the explosion. The SN light curve has a double-peak shape. It reached a first maximum of Mr = −19.6 ± 0.2 mag, fol ...
Leto: 2026 Vir: Univerza v Novi Gorici (UNG)
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