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researcher

M. H. M. Morais

4 papers here

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

author position
  • first author1
  • last author3

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP4
ORCID 0000-0001-5333-2736

identity via Semantic Scholar / OpenAlex

activity
20122023
most citedResonance capture at arbitrary inclination

48 citations · 77 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.EP2023★ 2 cited

A numerical study of fourth- and fifth-order retrograde mean motion resonances in planetary systems

Alan Cefali Signor, Gabriel Antonio Carita, Maria Helena Moreira Morais

We present a numerical study on the stability of all fourth- and fifth-order retrograde mean motion resonances (1/3, 3/1, 1/4, 4/1, 2/3, and 3/2) in the 3-body problem composed of…

astro-ph.EP2020★ 27 cited

An interstellar origin for high-inclination Centaurs

Fathi Namouni, Helena Morais

We investigate the possible origins of real high-inclination Centaurs and trans-neptunian objects using a high-resolution statistical search for stable orbits that simulates their…

astro-ph.EP2014★ 48 cited

Resonance capture at arbitrary inclination

Fathi Namouni, Maria Helena Moreira Morais

Resonance capture is studied numerically in the three-body problem for arbitrary inclinations. Massless particles are set to drift from outside the 1:5 resonance with a Jupiter-mas…

astro-ph.EP2012

Stellar wobble in triple star systems

M. H. M. Morais, A. C. M. Correia

The radial velocity method for detecting extra-solar planets relies on measuring the star's wobble around the system's center of mass. Since this is an indirect method, we may ask…

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