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researcher

P. Agrawal

14 papers hereh-index 9221 citations20 works total

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

author position
  • first author5
  • middle author8

Across the 13 of 14 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR9
  • astro-ph.GA2
  • astro-ph.HE2
  • astro-ph.IM1
same name
  • P. Agrawal — 51 papers, h 20
  • P. Agrawal — 47 papers, h 27
  • P. Agrawal — 33 papers, h 20
  • P. Agrawal — 11 papers, h 33
  • P. Agrawal — 5 papers, h 22
  • P. Agrawal — 4 papers, h 2

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
20202026
most citedBonn Optimized Stellar Tracks (BoOST). Simulated Populations of Massive and Very Massive Stars for Astrophysical Applications

63 citations · 238 across the 14 of their papers we have counts for

collaborators
Showing 2023Show all

3 papers · 1 filter

astro-ph.GA2023★ 3 cited

Young Star Clusters Dominate the Production of Detached Black Hole-Star Binaries

Ugo Niccolò Di Carlo, Poojan Agrawal, Carl L. Rodriguez +1

The recent discovery of two detached black hole-star (BH-star) binaries from Gaia's third data release has sparkled interest in understanding the formation mechanisms of these syst…

astro-ph.SR2023★ 12 cited

Modelling stellar evolution in mass-transferring binaries and gravitational-wave progenitors with METISSE

Poojan Agrawal, Jarrod Hurley, Simon Stevenson +3

Massive binaries are vital sources of various transient processes, including gravitational-wave mergers. However, large uncertainties in the evolution of massive stars, both physic…

astro-ph.SR2023★ 10 cited

Bringing Stellar Evolution & Feedback Together: Summary of proposals from the Lorentz Center Workshop, 2022

Sam Geen, Poojan Agrawal, Paul A. Crowther +34

Stars strongly impact their environment, and shape structures on all scales throughout the universe, in a process known as ``feedback''. Due to the complexity of both stellar evolu…

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