Evolution of migrating planet pairs in resonance (2003)
- Authors:
- USP affiliated authors: MELLO, SYLVIO FERRAZ DE - IAG ; MICHTCHENKO, TATIANA ALEXANDROVNA - IAG
- Unidade: IAG
- Assunto: MECÂNICA CELESTE
- Language: Inglês
- Imprenta:
- Source:
- Título: Celestial Mechanics and Dynamical Astronomy
- ISSN: 0035-8711
- Volume/Número/Paginação/Ano: v.87, p. 99-112, 2003
-
ABNT
FERRAZ-MELLO, Sylvio e BEAUGÉ, C e MICHTCHENKO, Tatiana Alexandrovna. Evolution of migrating planet pairs in resonance. Celestial Mechanics and Dynamical Astronomy, v. 87, p. 99-112, 2003Tradução . . Acesso em: 04 mar. 2026. -
APA
Ferraz-Mello, S., Beaugé, C., & Michtchenko, T. A. (2003). Evolution of migrating planet pairs in resonance. Celestial Mechanics and Dynamical Astronomy, 87, 99-112. -
NLM
Ferraz-Mello S, Beaugé C, Michtchenko TA. Evolution of migrating planet pairs in resonance. Celestial Mechanics and Dynamical Astronomy. 2003 ;87 99-112.[citado 2026 mar. 04 ] -
Vancouver
Ferraz-Mello S, Beaugé C, Michtchenko TA. Evolution of migrating planet pairs in resonance. Celestial Mechanics and Dynamical Astronomy. 2003 ;87 99-112.[citado 2026 mar. 04 ] - Dynamic picture of the inner asteroid belt: implications for the density, size and taxonomic distributions of real objects
- On the V-type asteroids outside the Vesta family I. Interplay of nonlinear secular resonances and the Yakovsky effect: the cases of 956 Elisa and 809 Lundia
- Origin of the Basaltic Asteroid 1459 Magnya: A Dynamical and Mineralogical Study of the Outer Main Belt
- Dynamic portrait of the planetary 2/1 mean-motion resonace: I. systems with a more massive outer planet
- Dynamics of two planets in the 2:1 and 3:2 ressonances
- Resonant Structure of the outer solar system in the neighborhood of the planets
- Determinação da órbita de exoplanetas com inferência estatística
- Study of diffusive phenomena within 2/1 and 3/2 asteroidal resonances
- Determination of dynamical and physical parameters of the system CoRoT 3
- The role of close encounters with (4) Vesta in the origin of the basaltic NEAs
How to cite
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
