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S. K. Jeena

4 papers here

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author2
  • middle author1
  • last author1

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR4

identity via Semantic Scholar / OpenAlex

activity
20232025
most citedThe Occurrence and Impact of Carbon-Oxygen Shell Mergers in Massive Stars

13 citations · 14 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.SR2025

Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors

Archana Purushothaman, Arkaprabha Sarangi, S. K. Jeena

Core-collapse supernovae (CCSNe) are among the primary sources of dust in galaxies. In this study, we derive theoretical upper limits on dust masses as a function of supernova (SN)…

astro-ph.SR2025★ 13 cited

The Occurrence and Impact of Carbon-Oxygen Shell Mergers in Massive Stars

L. Roberti, M. Pignatari, H. E. Brinkman +6

In their final stages before undergoing a core-collapse supernova, massive stars may experience mergers between internal shells where carbon (C) and oxygen (O) are consumed as fuel…

astro-ph.SR2024

Origin of α-Poor Very Metal-Poor Stars

S. K. Jeena, Projjwal Banerjee

Among very metal-poor (VMP) stars, α-poor VMP (αPVMP) stars that have sub-solar values of [X/Fe] for Mg and other α elements are rare and are thought to have been for…

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 ∼140--260M⊙​ are expected to end their lives as pair-instability supernovae (PISNe). The abundance p…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.