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Tom Abel

Kavli Institute for Particle Astrophysics and Cosmology, Stanford, SLAC

132 papers hereh-index 6516.5k citations211 works total

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

author position
  • sole author2
  • first author12
  • middle author54
  • last author59

Across the 127 of 132 papers where every author was matched, so the position is known.

fields
  • astro-ph66
  • astro-ph.CO40
  • astro-ph.GA8
  • astro-ph.IM6
  • astro-ph.SR4
  • physics.comp-ph4
affiliations
  • Kavli Institute for Particle Astrophysics and Cosmology, Stanford, SLAC
Homepage
same name
  • Tom Abel — 14 papers, h 7
  • Tom Abel — 8 papers, h 5
  • Tom Abel — 3 papers
  • Tom Abel — 3 papers, h 3
  • Tom Abel — 2 papers, h 2
  • Tom Abel — 2 papers, h 3

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
19962023
most citedA Multi-Code Analysis Toolkit for Astrophysical Simulation Data

1.2k citations · 18.2k across the 129 of their papers we have counts for

collaborators
Showing 2008Show all

4 papers · 1 filter

astro-ph2008★ 64 cited

Connecting Reionization to the Local Universe

Marcelo A. Alvarez, Michael T. Busha, Tom Abel +1

We present results of combined N-body and three-dimensional reionization calculations to determine the relationship between reionization history and local environment in a volume 1…

astro-ph2008★ 282 cited

Accretion onto the First Stellar Mass Black Holes

Marcelo A. Alvarez, John H. Wise, Tom Abel

The first stars in the universe, forming at redshifts z>15 in minihalos with masses of order 10^6 Msun, may leave behind black holes as their remnants. These objects could conceiva…

astro-ph2008

Resolving the Formation of Protogalaxies

John H. Wise

Cosmic structure originated from minute density perturbations in an almost homogeneous universe. The first stars are believed to be very massive and luminous, providing the first i…

astro-ph2008★ 272 cited

Uncertainties in H2 and HD Chemistry and Cooling and their Role in Early Structure Formation

S. C. O. Glover, T. Abel

At low temperatures, the main coolant in primordial gas is molecular hydrogen, H2. Recent work has shown that primordial gas that is not collapsing gravitationally but is cooling f…

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