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researcher

E. Moreno

3 papers hereh-index 6207 citations13 works total

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

author position
  • last author1

Across the 1 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA2
  • astro-ph1
same name
  • E. Moreno — 69 papers, h 44
  • E. Moreno — 46 papers, h 20
  • E. Moreno — 39 papers, h 13
  • E. Moreno — 28 papers, h 13
  • E. Moreno — 19 papers, h 29
  • E. Moreno — 19 papers, h 6

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
20062016
most citedUnderstanding the spiral structure of the Milky Way using the local kinematic groups

119 citations · 175 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.GA2016★ 18 cited

On the Origin of High-Altitude Open Clusters in the Milky Way

L. A. Martinez-Medina, B. Pichardo, E. Moreno +2

We present a dynamical study of the effect of the bar and spiral arms on the simulated orbits of open clusters in the Galaxy. Specifically, this work is devoted to the puzzling pre…

astro-ph.GA2011★ 119 cited

Understanding the spiral structure of the Milky Way using the local kinematic groups

T. Antoja, F. Figueras, M. Romero-Gómez +3

We study the spiral arm influence on the solar neighbourhood stellar kinematics. As the nature of the Milky Way (MW) spiral arms is not completely determined, we study two models:…

astro-ph2006★ 38 cited

The X-ray binary 2S0114+650=LSI+65 010:A slow pulsar or tidally-induced pulsations?

G. Koenigsberger, L. Georgiev, E. Moreno +3

The X-ray source 2S0114+650=LSI+65 010 is a binary system containing a B-type primary and a low mass companion believed to be a neutron star. The system has three reported periodic…

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