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researcher

A. Heger

78 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 author5
  • middle author38
  • last author19

Across the 62 of 78 papers where every author was matched, so the position is known.

fields
  • astro-ph27
  • astro-ph.HE23
  • astro-ph.SR15
  • astro-ph.GA9
  • astro-ph.IM2
  • nucl-ex2
same name
  • A. Heger — 14 papers, h 18
  • A. Heger — 8 papers, h 6
  • A. Heger — 7 papers, h 10
  • A. Heger — 5 papers, h 6
  • A. Heger — 3 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
19972021
most citedThe Supernova -- Gamma-Ray Burst Connection

1.8k citations · 5.7k across the 38 of their papers we have counts for

collaborators
Showing 2005Show all

4 papers · 1 filter

astro-ph2005

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

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

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

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.