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20122026
most citedThree-Dimensional Simulations of Neutrino-Driven Core-Collapse Supernovae from Low-Mass Single and Binary Star Progenitors

215 citations · 830 across the 26 of their papers we have counts for

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13 papers · 1 filter

astro-ph.SR2026

Super-Chandrasekhar white dwarfs by the evolution of magnetized main-sequence stars: New mass-limits from STARS simulation

Zenia Zuraiq, Banibrata Mukhopadhyay, Achal Kumar +4

We explore the time evolution of the magnetized main-sequence stars (MSs) to magnetized non-rotating white dwarfs (WDs) with a series of models, capturing modified Hertzsprung-Russ…

astro-ph.SR2024

Origin of -Poor Very Metal-Poor Stars

S. K. Jeena, Projjwal Banerjee

Among very metal-poor (VMP) stars, -poor VMP (PVMP) stars that have sub-solar values of for Mg and other elements are rare and are thought to have been for…

astro-ph.SR2024★ 1 cited

SDSSJ0018-0939: A Clear Signature of Sub-Chandrasekhar Mass Type 1a Supernova

S. K. Jeena, Projjwal Banerjee

Very metal-poor (VMP) stars () that have sub-solar values of for elements such as Mg, Si, and Ca, are referred to as -poor VMP stars. The…

astro-ph.SR2024★ 3 cited

Origin of LAMOST J1010+2358 Revisited

S. K. Jeena, Projjwal Banerjee

Signature from Pop III massive stars of -- that end their lives as pair-instability supernovae (PISNe) are expected to be seen in very metal-poor (VMP) sta…

astro-ph.SR2023★ 1 cited

On the Core-Collapse Supernova Explanation for LAMOST J1010+2358

S K Jeena, Projjwal Banerjee, Alexander Heger

Low-metallicity very massive stars with an initial mass of -- are expected to end their lives as pair-instability supernovae (PISNe). The abundance p…

astro-ph.SR2023

Rapidly Rotating Massive Pop III stars: A Solution for High Carbon Enrichment in CEMP-no Stars

Jeena S K, Projjwal Banerjee, Gen Chiaki +1

Very metal-poor stars that have and that are enhanced in C relative to Fe () but have no enhancement of heavy elements ($[\text…