Galactic corotation as a principal "driver'' for the formation of bimodal abundance radial distribution in the disk of our Galaxy (2012)
- Authors:
- Autor USP: LEPINE, JACQUES RAYMOND DANIEL - IAG
- Unidade: IAG
- Subjects: ESTRELAS; GALÁXIA (VIA LÁCTEA); ESTRUTURA DA GALÁXIA; ABUNDÂNCIAS (ASTRONOMIA)
- Language: Inglês
- Imprenta:
- Source:
- Título: Astronomical & Astrophysical Transactions
- ISSN: 1055-6796
- Volume/Número/Paginação/Ano: v. 27, n. 2, p. 359-364, 2012
-
ABNT
ACHAROVA, I. A e LÉPINE, Jacques Raymond Daniel e MISHUROV, Yu. N. Galactic corotation as a principal "driver'' for the formation of bimodal abundance radial distribution in the disk of our Galaxy. Astronomical & Astrophysical Transactions, v. 27, n. 2, p. 359-364, 2012Tradução . . Acesso em: 12 jan. 2026. -
APA
Acharova, I. A., Lépine, J. R. D., & Mishurov, Y. N. (2012). Galactic corotation as a principal "driver'' for the formation of bimodal abundance radial distribution in the disk of our Galaxy. Astronomical & Astrophysical Transactions, 27( 2), 359-364. -
NLM
Acharova IA, Lépine JRD, Mishurov YN. Galactic corotation as a principal "driver'' for the formation of bimodal abundance radial distribution in the disk of our Galaxy. Astronomical & Astrophysical Transactions. 2012 ; 27( 2): 359-364.[citado 2026 jan. 12 ] -
Vancouver
Acharova IA, Lépine JRD, Mishurov YN. Galactic corotation as a principal "driver'' for the formation of bimodal abundance radial distribution in the disk of our Galaxy. Astronomical & Astrophysical Transactions. 2012 ; 27( 2): 359-364.[citado 2026 jan. 12 ] - The role of resonances in the evolution of galactic disks
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- A galactic ring of minimum stellar density near the solar orbit radius
- Models for the 3D axisymmetric gravitational potential of the Milky Way galaxy: a detailed modelling of the Galactic disk
- Galactic corotation as a principal "driver'' for the formation of bimodal abundance radial distribution in the disk of our Galaxy
- The galactic abundance gradient from cepheids V. transition zone between 10 and 11 kpc
- Open cluster radial velocity determination from observations at Observatório Pico Dos Dias
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