On the similarities and differences between 3/2 and 2/1 asteroidal resonances (1999)
- Authors:
- USP affiliated authors: MICHTCHENKO, TATIANA ALEXANDROVNA - IAG ; MELLO, SYLVIO FERRAZ DE - IAG
- Unidade: IAG
- Subjects: ASTRONOMIA; ASTROFÍSICA SOLAR
- Language: Inglês
- Imprenta:
- Source:
-
ABNT
MICHTCHENKO, Tatiana Alexandrovna e FERRAZ-MELLO, Sylvio. On the similarities and differences between 3/2 and 2/1 asteroidal resonances. The dynamics of small bodies in the solar system : a major key to solar system studies. Tradução . Dordrecht: Kluwer, 1999. . . Acesso em: 11 mar. 2026. -
APA
Michtchenko, T. A., & Ferraz-Mello, S. (1999). On the similarities and differences between 3/2 and 2/1 asteroidal resonances. In The dynamics of small bodies in the solar system : a major key to solar system studies. Dordrecht: Kluwer. -
NLM
Michtchenko TA, Ferraz-Mello S. On the similarities and differences between 3/2 and 2/1 asteroidal resonances. In: The dynamics of small bodies in the solar system : a major key to solar system studies. Dordrecht: Kluwer; 1999. [citado 2026 mar. 11 ] -
Vancouver
Michtchenko TA, Ferraz-Mello S. On the similarities and differences between 3/2 and 2/1 asteroidal resonances. In: The dynamics of small bodies in the solar system : a major key to solar system studies. Dordrecht: Kluwer; 1999. [citado 2026 mar. 11 ] - 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
