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20152026
most citedPulsational Pair-Instability Model for Superluminous Supernova PTF12dam: Interaction and Radioactive Decay

37 citations · 160 across the 12 of their papers we have counts for

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15 papers · 1 filter

astro-ph.HE2026

Helium superluminous SN 2021bnw : an explosion of a massive star with a pre-outburst

Alexandra Kozyreva, Matteo Bugli, Alexey Mironov +1

Superluminous supernovae (SLSNe) remain an intriguing topic in supernova (SN) transient astronomy. While the majority of SLSNe are shown to be explained by energy streaming from th…

astro-ph.HE2026

The nearby He-rich superluminous supernova SN 2021bnw during photospheric phases

A. Fiore, A. Kozyreva, L. Yan +40

Aim. We present and interpret the data of the nearby hydrogen-deficient but helium-rich superluminous supernova SN 2021bnw which reached a magnitude of -20.7 at maximum luminosity…

astro-ph.HE2024★ 15 cited

SN 2023ixf -- an average-energy explosion with circumstellar medium and a precursor

Alexandra Kozyreva, Andrea Caputo, Petr Baklanov +2

Abridged: The fortunate proximity of the SN2023ixf allowed astronomers to follow its evolution from almost the moment of the collapse of the progenitor's core. SN2023ixf can be exp…

astro-ph.HE2024★ 1 cited

Primary and secondary source of energy in the superluminous supernova 2018ibb

Alexandra Kozyreva, Luke Shingles, Petr Baklanov +2

We examine the pair-instability origin of superluminous supernova 2018ibb. As the base model, we use a non-rotating stellar model with an initial mass of 250 Msun at about 1/15 sol…

astro-ph.HE2022★ 20 cited

The circumstellar material around the Type IIP SN 2021yja

Alexandra Kozyreva, Jakub Klencki, Alexei V. Filippenko +4

The majority of Type II-plateau supernovae (SNe IIP) have light curves that are not compatible with the explosions of stars in a vacuum; instead, the light curves require the proge…

astro-ph.HE2021

Parameters of the type-IIP supernova SN 2012aw

A. A. Nikiforova, P. V. Baklanov, S. I. Blinnikov +7

We present the results the photometric observations of the Type IIP supernova SN 2012aw obtained for the time interval from 7 till 371 days after the explosion. Using the previousl…