Modeling close encouters with massive asteroids: a Markovian approach. An aplication to the Vesta family (2007)
- Autores:
- Autores USP: MICHTCHENKO, TATIANA ALEXANDROVNA - IAG ; MELLO, SYLVIO FERRAZ DE - IAG
- Unidade: IAG
- Assuntos: MECÂNICA CELESTE; ASTEROIDES; PLANETAS MENORES
- Idioma: Inglês
- Imprenta:
- Fonte:
- Título do periódico: Astronomy and Astrophysics
- ISSN: 0004-6361
- Volume/Número/Paginação/Ano: v.465, n.1, p. 315-330, 2007
-
ABNT
CARRUBA, V et al. Modeling close encouters with massive asteroids: a Markovian approach. An aplication to the Vesta family. Astronomy and Astrophysics, v. 465, n. 1, p. 315-330, 2007Tradução . . Acesso em: 11 maio 2024. -
APA
Carruba, V., Michtchenko, T. A., Ferraz-Mello, S., Roig, F., & Nesvorný, D. (2007). Modeling close encouters with massive asteroids: a Markovian approach. An aplication to the Vesta family. Astronomy and Astrophysics, 465( 1), 315-330. -
NLM
Carruba V, Michtchenko TA, Ferraz-Mello S, Roig F, Nesvorný D. Modeling close encouters with massive asteroids: a Markovian approach. An aplication to the Vesta family. Astronomy and Astrophysics. 2007 ;465( 1): 315-330.[citado 2024 maio 11 ] -
Vancouver
Carruba V, Michtchenko TA, Ferraz-Mello S, Roig F, Nesvorný D. Modeling close encouters with massive asteroids: a Markovian approach. An aplication to the Vesta family. Astronomy and Astrophysics. 2007 ;465( 1): 315-330.[citado 2024 maio 11 ] - Planetary masses and orbital parameters from radial velocity measurements
- Dynamical maps of the inner asteroid belt
- Júpiters, Netunos e super-terras quentes
- Detectability and error estimation in orbital fits of resonant extrasolar planets
- Retrato dinâmico do cinturão asteroidal interior
- Detectability and error estimation in orbital fits of resonant extrasolar planets
- Dynamics of two planets in the 2:1 and 3:2 mean motion resonances
- On the depletion of the Hecuba gap in the asteroidal belt
- 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: II. systems with a more massive inner planet
Como citar
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas