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P. Banerjee

26 papers hereh-index 11641 citations40 works total

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

author position
  • first author9
  • middle author12
  • last author4

Across the 25 of 26 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR13
  • astro-ph.GA6
  • astro-ph.HE5
  • astro-ph.IM1
  • nucl-th1
same name
  • P. Banerjee — 93 papers
  • P. Banerjee — 50 papers, h 60
  • P. Banerjee — 31 papers, h 15
  • P. Banerjee — 18 papers, h 10
  • P. Banerjee — 12 papers, h 10
  • P. Banerjee — 9 papers, h 14

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
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

collaborators
Showing 2024Show all

4 papers · 1 filter

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.GA2024★ 2 cited

Can supernova from runaway stars mimic the signs of absorbing `super-virial' gas?

Mukesh Singh Bisht, Projjwal Banerjee, Biman B. Nath +1

The recent detection of large column density absorption lines from highly ionized gas in a few directions through the circumgalactic medium (CGM) of the Milky Way (MW) has been puz…

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 ([Fe/H]≤−2) that have sub-solar values of [X/Fe] for α elements such as Mg, Si, and Ca, are referred to as α-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 140--260M⊙​ that end their lives as pair-instability supernovae (PISNe) are expected to be seen in very metal-poor (VMP) sta…

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