Carbon star envelopes: near-ir photometry, mas loss and evolutionary status of a sample of iras stars (1990)
- Authors:
- Autor USP: LEPINE, JACQUES RAYMOND DANIEL - IAG
- Unidade: IAG
- Assunto: ASTRONOMIA
- Language: Inglês
- Imprenta:
- Source:
- Título: Astronomy and Astrophysics
- Volume/Número/Paginação/Ano: v. 227, n. 1 , p. 82-104, jan. 1990
-
ABNT
EPCHTEIN, N e LE BERTRE, T e LÉPINE, Jacques Raymond Daniel. Carbon star envelopes: near-ir photometry, mas loss and evolutionary status of a sample of iras stars. Astronomy and Astrophysics, v. 227, n. ja 1990, p. 82-104, 1990Tradução . . Acesso em: 24 jan. 2026. -
APA
Epchtein, N., Le Bertre, T., & Lépine, J. R. D. (1990). Carbon star envelopes: near-ir photometry, mas loss and evolutionary status of a sample of iras stars. Astronomy and Astrophysics, 227( ja 1990), 82-104. -
NLM
Epchtein N, Le Bertre T, Lépine JRD. Carbon star envelopes: near-ir photometry, mas loss and evolutionary status of a sample of iras stars. Astronomy and Astrophysics. 1990 ; 227( ja 1990): 82-104.[citado 2026 jan. 24 ] -
Vancouver
Epchtein N, Le Bertre T, Lépine JRD. Carbon star envelopes: near-ir photometry, mas loss and evolutionary status of a sample of iras stars. Astronomy and Astrophysics. 1990 ; 227( ja 1990): 82-104.[citado 2026 jan. 24 ] - Construção de um catálogo de aglomerados abertos para estudo da dinâmica da estrutura espiral da galáxia
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- New catalogue of optically visible open clusters and candidates
- Constraints on the mass of the dark halo from the rotation curve of the galaxy
- A velocidade da rotação dos braços espirais da Via Láctea
- Fractal 3-d simulations of molecular clouds
- Model of the galaxy for predicting star counts in the infrared
- Models for the 3D axisymmetric gravitational potential of the Milky Way galaxy: a detailed modelling of the Galactic disk
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