On the current distribution of main belt objects: constraints for evolutionary models (2016)
- Authors:
- USP affiliated author: MICHTCHENKO, TATIANA ALEXANDROVNA - IAG
- School: IAG
- DOI: 10.1051/0004-6361/201525754
- Subjects: PLANETAS MENORES; ASTEROIDES; ANÁLISE DE DADOS; MECÂNICA CELESTE
- Language: Inglês
- Imprenta:
- Source:
- Título do periódico: Astronomy & Astrophysics
- ISSN: 0004-6361
- Volume/Número/Paginação/Ano: v. 588, p. A11/1-A11/26, 2016
- Este periódico é de assinatura
- Este artigo é de acesso aberto
- URL de acesso aberto
- Cor do Acesso Aberto: bronze
-
ABNT
MICHTCHENKO, Tatiana Alexandrovna; LAZZARO, D; CARVANO, J. M. On the current distribution of main belt objects: constraints for evolutionary models. Astronomy & Astrophysics, Les Ulis, v. 588, p. A11/1-A11/26, 2016. Disponível em: < http://dx.doi.org/10.1051/0004-6361/201525754 > DOI: 10.1051/0004-6361/201525754. -
APA
Michtchenko, T. A., Lazzaro, D., & Carvano, J. M. (2016). On the current distribution of main belt objects: constraints for evolutionary models. Astronomy & Astrophysics, 588, A11/1-A11/26. doi:10.1051/0004-6361/201525754 -
NLM
Michtchenko TA, Lazzaro D, Carvano JM. On the current distribution of main belt objects: constraints for evolutionary models [Internet]. Astronomy & Astrophysics. 2016 ; 588 A11/1-A11/26.Available from: http://dx.doi.org/10.1051/0004-6361/201525754 -
Vancouver
Michtchenko TA, Lazzaro D, Carvano JM. On the current distribution of main belt objects: constraints for evolutionary models [Internet]. Astronomy & Astrophysics. 2016 ; 588 A11/1-A11/26.Available from: http://dx.doi.org/10.1051/0004-6361/201525754 - Estabilidade das órbitas planetárias nos sistemas de estrelas binárias
- Modelagem do movimento planetário nos sistemas de estrelas múltiplas
- Stability and dynamics of terrestrial planets in binary star systems: application on Alpha Centauri
- Dynamics of the 3:1 resonant planetary systems
- Dynamics of the 3/1 planetary mean-motion resonance: an application to the HD60532 b-c planetary system
- The use of the Mathematica software in the study of planetary dynamics
- Modelling the secular evolution of migrating planet pairs
- A new scenario for the origin of the 3/2 resonant system HD 45364
- Adapting a gas accretion scenario for migrating planets in FARGO3D
- Adapting a solid accretion scenario for migrating planets in FARGO3D
Informações sobre o DOI: 10.1051/0004-6361/201525754 (Fonte: oaDOI API)
How to cite
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
