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E. Noyola

22 papers hereh-index 211.6k citations43 works total

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

author position
  • first author3
  • middle author13
  • last author1

Across the 17 of 22 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA14
  • astro-ph3
  • astro-ph.HE3
  • astro-ph.IM2
same name
  • E. Noyola — 1 paper, 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
20052021
most citedSurface Brightness Profiles of Galactic Globular Clusters from Hubble Space Telescope Images

155 citations · 1.5k across the 22 of their papers we have counts for

collaborators
Showing 2012Show all

3 papers · 1 filter

astro-ph.GA2012★ 113 cited

Limits on intermediate-mass black holes in six Galactic globular clusters with integral-field spectroscopy

Nora Lützgendorf, Markus Kissler-Patig, Karl Gebhardt +6

The formation of supermassive black holes at high redshift still remains a puzzle to astronomers. Their growth becomes reasonable only when starting from a massive seed black hole…

astro-ph.GA2012★ 28 cited

High-velocity stars in the cores of globular clusters: The illustrative case of NGC 2808

Nora Lützgendorf, Alessia Gualandris, Markus Kissler-Patig +7

We report the detection of five high-velocity stars in the core of the globular cluster NGC 2808. The stars lie on the the red giant branch and show total velocities between 40 and…

astro-ph.GA2012★ 43 cited

Central kinematics of the globular cluster NGC 2808: Upper limit on the mass of an intermediate-mass black hole

Nora Lützgendorf, Markus Kissler-Patig, Karl Gebhardt +5

Globular clusters are an excellent laboratory for stellar population and dynamical research. Recent studies have shown that these stellar systems are not as simple as previously as…

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