Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: PLANETAS MENORES, ASTEROIDES, MECÂNICA CELESTE
ABNT
CARRUBA, V e MICHTCHENKO, Tatiana Alexandrovna. A frequency approach to identifying asteroid families: II. Families interacting with nonlinear secular resonances and low-order mean-motion resonances. Astronomy & Astrophysics, v. 493, p. 267-282, 2009Tradução . . Acesso em: 15 jul. 2025.APA
Carruba, V., & Michtchenko, T. A. (2009). A frequency approach to identifying asteroid families: II. Families interacting with nonlinear secular resonances and low-order mean-motion resonances. Astronomy & Astrophysics, 493, 267-282.NLM
Carruba V, Michtchenko TA. A frequency approach to identifying asteroid families: II. Families interacting with nonlinear secular resonances and low-order mean-motion resonances. Astronomy & Astrophysics. 2009 ; 493 267-282.[citado 2025 jul. 15 ]Vancouver
Carruba V, Michtchenko TA. A frequency approach to identifying asteroid families: II. Families interacting with nonlinear secular resonances and low-order mean-motion resonances. Astronomy & Astrophysics. 2009 ; 493 267-282.[citado 2025 jul. 15 ]