SN 2021wvw: A core-collapse supernova at the sub-luminous, slower, and shorter end of Type IIPs
Rishabh Singh Teja, Jared A. Goldberg, D. K. Sahu, G. C. Anupama,, Avinash Singh, Vishwajeet Swain, and Varun Bhalerao

TL;DR
SN 2021wvw is a rare, sub-luminous Type IIP supernova with a short plateau, low velocity, and low nickel mass, providing insights into diverse core-collapse supernovae and their progenitors.
Contribution
This study presents detailed observations and modeling of SN 2021wvw, a unique low-luminosity, short-plateau Type IIP supernova, expanding understanding of supernova diversity and progenitor characteristics.
Findings
SN 2021wvw has a short 75-day plateau and sharp transition to the tail phase.
It has a peak magnitude of -16.1 mag and nickel mass of 0.020 Msol.
Hydrodynamical modeling suggests a low-metallicity, high-mass RSG progenitor with significant fallback.
Abstract
We present detailed multi-band photometric and spectroscopic observations and analysis of a rare core-collapse supernova SN 2021wvw, that includes photometric evolution up to 250 d and spectroscopic coverage up to 100 d post-explosion. A unique event that does not fit well within the general trends observed for Type II-P supernovae, SN 2021wvw shows an intermediate luminosity with a short plateau phase of just about 75 d, followed by a very sharp (~10 d) transition to the tail phase. Even in the velocity space, it lies at a lower velocity compared to a larger Type II sample. The observed peak absolute magnitude is -16.1 mag in r-band, and the nickel mass is well constrained to 0.020(6) Msol. Detailed hydrodynamical modeling using MESA+STELLA suggests a radially compact, low-metallicity, high-mass Red Supergiant progenitor (ZAMS mass=18 Msol), which exploded with ~0.2e51 erg/s leaving an…
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Taxonomy
TopicsGamma-ray bursts and supernovae
