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researcher

A. Heger

171 papers hereh-index 5920.4k citations356 works total

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

author position
  • first author12
  • middle author94
  • last author49

Across the 155 of 171 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE57
  • astro-ph.SR50
  • astro-ph37
  • astro-ph.GA13
  • astro-ph.CO9
  • nucl-ex3
same name
  • A. Heger — 27 papers, h 18
  • A. Heger — 14 papers, h 6
  • A. Heger — 12 papers, h 10
  • A. Heger — 11 papers, h 6
  • A. Heger — 11 papers, h 2
  • A. Heger — 1 paper, h 1

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
19972023
most citedHow Massive Single Stars End their Life

2.2k citations · 21.5k across the 170 of their papers we have counts for

collaborators
Showing 2005 · astro-phShow all

4 papers · 2 filters

astro-ph2005★ 4 cited

Detecting Primordial Stars

Evan Scannapieco, Andrea Ferrara, Alexander Heger +3

We study the detectability of primordial metal-free stars. Cosmological enrichment is a local process that takes place over an extended redshift range. While the duration of this t…

astro-ph2005★ 941 cited

The Progenitor Stars of Gamma-Ray Bursts

Stan Woosley, Alexander Heger

Those massive stars that, during their deaths, give rise to gamma-ray bursts (GRBs) must be endowed with an unusually large amount of angular momentum in their inner regions, one t…

astro-ph2005★ 153 cited

The Detectability of Pair-Production Supernovae at z < 6

Evan Scannapieco, Piero Madau, Stan Woosley +2

Nonrotating, zero metallicity stars with initial masses 140 < M < 260 solar masses are expected to end their lives as pair-production supernovae (PPSNe), in which an electron-posit…

astro-ph2005★ 154 cited

Which Massive stars are Gamma-Ray Burst Progenitors?

Jelena Petrovic, Norbert Langer, Sung-Chul Yoon +1

The collapsar model for gamma-ray bursts requires three essential ingredients: a massive core, removal of the hydrogen envelope, and enough angular momentum in the core. We study c…

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