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researcher

A. Geller

67 papers hereh-index 272k citations110 works total

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

author position
  • first author16
  • middle author32
  • last author15

Across the 63 of 67 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR56
  • astro-ph.EP4
  • astro-ph.GA3
  • astro-ph.HE2
  • astro-ph1
  • astro-ph.IM1
same name
  • A. Geller — 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
20082025
most citedAge and helium content of the open cluster NGC 6791 from multiple eclipsing binary members. II. age dependencies and new insights

181 citations · 2.8k across the 66 of their papers we have counts for

collaborators
Showing 2013Show all

3 papers · 1 filter

astro-ph.SR2013★ 46 cited

Consequences of Dynamical Disruption and Mass Segregation for the Binary Frequencies of Star Clusters

Aaron M. Geller, Richard de Grijs, Chengyuan Li +1

The massive (13,000-26,000 Msolar), young (15-30 Myr) Large Magellanic Cloud star cluster NGC 1818 reveals an unexpected increasing binary frequency with radius for F-type stars (1…

astro-ph.SR2013★ 46 cited

WOCS 40007: A Detached Eclipsing Binary near the Turnoff of the Open Cluster NGC 6819

Mark W. Jeffries, Eric L. Sandquist, Robert D. Mathieu +10

We analyze extensive BVR_cI_c time-series photometry and radial-velocity measurements for WOCS 40007 (Auner 259; KIC 5113053), a double-lined detached eclipsing binary and a member…

astro-ph.SR2013★ 66 cited

The Dynamical Significance of Triple Star Systems in Star Clusters

Nathan W. C. Leigh, Aaron M. Geller

Over the last few decades, observational surveys have revealed that high-order multiple-star systems (e.g. triples, quadruples, etc.), and triples in particular, are common in our…

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