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N. Cuello

34 papers hereh-index 15515 citations37 works total

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

author position
  • first author2
  • middle author29

Across the 31 of 34 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP25
  • astro-ph.SR7
  • astro-ph.GA1
  • astro-ph.IM1
same name
  • N. Cuello — 76 papers, h 16

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
20182026
most citedFlybys in protoplanetary discs: I. Gas and dust dynamics

142 citations · 809 across the 32 of their papers we have counts for

collaborators
Showing 2019Show all

4 papers · 1 filter

astro-ph.EP2019★ 29 cited

Dusty clumps in circumbinary discs

Pedro P. Poblete, Nicolás Cuello, Jorge Cuadra

Recent observations have revealed that protoplanetary discs often exhibit cavities and azimuthal asymmetries such as dust traps and clumps. The presence of a stellar binary system…

astro-ph.EP2019★ 30 cited

Ploonets: formation, evolution and detectability of tidally detached exomoons

Mario Sucerquia, Jaime A. Alvarado-Montes, Jorge I. Zuluaga +2

Close-in giant planets represent the most significant evidence of planetary migration. If large exomoons form around migrating giant planets which are more stable (e.g. those in th…

astro-ph.EP2019★ 53 cited

Planet formation and stability in polar circumbinary discs

Nicolás Cuello, Cristian A. Giuppone

Context. Dynamical studies suggest that most circumbinary discs (CBDs) should be coplanar. However, some theoretical works show that under certain conditions a CBD can become polar…

astro-ph.EP2019★ 47 cited

Thermal torque effects on the migration of growing low-mass planets

O. M. Guilera, N. Cuello, M. Montesinos +4

As planets grow the exchange of angular momentum with the gaseous component of the protoplanetary disc produces a net torque resulting in a variation of the semi-major axis of the…

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