Zobrazeno 1 - 10
of 31
pro vyhledávání: '"M. H. M. Morais"'
Autor:
M. H. M. Morais, Fathi Namouni
Publikováno v:
Scopus
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
Computational and Applied Mathematics
Computational and Applied Mathematics, Springer Verlag, 2016, 35 (3), pp.881-891. ⟨10.1007/s40314-015-0295-3⟩
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
Computational and Applied Mathematics
Computational and Applied Mathematics, Springer Verlag, 2016, 35 (3), pp.881-891. ⟨10.1007/s40314-015-0295-3⟩
We start by reviewing our previous work on retrograde orbital configurations and on modeling and identifying retrograde resonances. Then, we present new results regarding the enhanced stability of retrograde configurations with respect to prograde co
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::58fb7d063f59dfb839e08611d7e94d29
http://arxiv.org/abs/2206.04628
http://arxiv.org/abs/2206.04628
Publikováno v:
Celestial Mechanics and Dynamical Astronomy
Celestial Mechanics and Dynamical Astronomy, Springer Verlag, 2021, 133 (5), ⟨10.1007/s10569-021-10020-0⟩
Scopus
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
Celestial Mechanics and Dynamical Astronomy, Springer Verlag, 2021, 133 (5), ⟨10.1007/s10569-021-10020-0⟩
Scopus
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
We describe the families of periodic orbits in the 2-dimensional 1/2 retrograde resonance at mass ratio 0.001, analyzing their stability and bifurcations into 3-dimensional periodic orbits. We explain the role played by periodic orbits in adiabatic r
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3bdb37e37e696613e829b9ea1a065dc9
https://hal.archives-ouvertes.fr/hal-03384544
https://hal.archives-ouvertes.fr/hal-03384544
Autor:
M. H. M. Morais, Fathi Namouni
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2020, 493 (2), pp.2854-2871. ⟨10.1093/mnras/staa348⟩
Web of Science
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2020, 493 (2), pp.2854-2871. ⟨10.1093/mnras/staa348⟩
Web of Science
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
We apply the analytical disturbing function for arbitrary inclination derived in our previous work to characterize resonant width and libration of mean motion resonances at arbitrary inclination obtained from direct numerical simulations of the three
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::16363a6bd95bce0e36fabffffe9c3141
http://arxiv.org/abs/2002.01832
http://arxiv.org/abs/2002.01832
Publikováno v:
Scopus
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
Made available in DSpace on 2022-04-28T19:47:46Z (GMT). No. of bitstreams: 0 Previous issue date: 2022-01-01 Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq) We study the dynamics of interior mean motion resonances of first, sec
Autor:
Fathi Namouni, M. H. M. Morais
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters
Monthly Notices of the Royal Astronomical Society: Letters, Oxford Journals, 2017, 472 (1), pp.L1-L4. ⟨10.1093/mnrasl/slx125⟩
Monthly Notices of the Royal Astronomical Society: Letters, Oxford Journals, 2017, 472 (1), pp.L1-L4. ⟨10.1093/mnrasl/slx125⟩
Capture in mean motion resonance has been observed in the Solar System for small objects with prograde as well as retrograde orbits of moderate inclinations. However, no example of an object with a nearly polar orbit was known to be in resonance with
Autor:
Fathi Namouni, M. H. M. Morais
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2017, 471 (2), pp.2097-2110. ⟨10.1093/mnras/stx1714⟩
Scopus
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2017, 471 (2), pp.2097-2110. ⟨10.1093/mnras/stx1714⟩
Scopus
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
The classical disturbing function of the three-body problem is based on an expansion of the gravitational interaction in the vicinity of nearly coplanar orbits. Consequently, it is not suitable for the identification and study of resonances of the Ce
Publikováno v:
Journal for Nature Conservation. 35:1-12
Invasion by alien plants results in serious adverse impacts on biodiversity, ecosystem services, economy and social welfare, and is an ever-increasing challenge for nature conservation. Control of established invasive species is frequently very diffi
Autor:
M. H. M. Morais, Fathi Namouni
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters
Monthly Notices of the Royal Astronomical Society: Letters, Oxford Journals, 2018, 477 (1), pp.L117-L121. ⟨10.1093/mnrasl/sly057⟩
Monthly Notices of the Royal Astronomical Society: Letters, Oxford Journals, 2018, 477 (1), pp.L117-L121. ⟨10.1093/mnrasl/sly057⟩
Asteroid (514107) 2015 BZ509 was discovered recently in Jupiter's co-orbital region with a retrograde motion around the Sun. The known chaotic dynamics of the outer Solar System have so far precluded the identification of its origin. Here, we perform
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::379b9f18152affca6c2ac3c37309147c
https://hal.archives-ouvertes.fr/hal-02398840
https://hal.archives-ouvertes.fr/hal-02398840
Autor:
Fathi Namouni, M. H. M. Morais
Publikováno v:
Web of Science
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2017, 467 (3), pp.2673-2683. ⟨10.1093/mnras/stx290⟩
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2017, 467 (3), pp.2673-2683. ⟨10.1093/mnras/stx290⟩
The effect of radial drift rate on mean motion resonance capture is studied for prograde, polar and retrograde orbits. We employ the numerical framework of our earlier exploration of resonance capture at arbitrary inclination. Randomly constructed sa
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9d842adfb68cb8259cb5c9b5f64a6813
Autor:
M. H. M. Morais, Fathi Namouni
Publikováno v:
Web of Science
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
Celestial Mechanics and Dynamical Astronomy
Celestial Mechanics and Dynamical Astronomy, Springer Verlag, 2016, 125 (1), pp.91-106. ⟨10.1007/s10569-016-9674-3⟩
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
Celestial Mechanics and Dynamical Astronomy
Celestial Mechanics and Dynamical Astronomy, Springer Verlag, 2016, 125 (1), pp.91-106. ⟨10.1007/s10569-016-9674-3⟩
Motivated by the dynamics of resonance capture, we study numerically the coorbital resonance for inclination180 >=I>=0 in the circular restricted three-body problem. We examine the similarities and differences between planar and three dimensional coo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1384ce79c76c196009289d0c471e5635
http://arxiv.org/abs/1602.04755
http://arxiv.org/abs/1602.04755