Grid of synthetic spectra for the determination of effective temperature, gravity and metallicity of f, g, and k stars: I. Description of the method

Grid of synthetic spectra for the determination of effective temperature, gravity and metallicity of f, g, and k stars: I. Description of the method (1991)

Authors:
Autor USP: BARBUY, BEATRIZ LEONOR SILVEIRA - IAG
Unidade: IAG
Assunto: ASTRONOMIA
Language: Inglês
Imprenta:
- Publisher place: New York
- Date published: 1991
Source:
- Título do periódico: Astronomy and Astrophysics
- Volume/Número/Paginação/Ano: v. 247, p. 108-121, 1991

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ABNT

CAYREL, R et al. Grid of synthetic spectra for the determination of effective temperature, gravity and metallicity of f, g, and k stars: I. Description of the method. Astronomy and Astrophysics, v. 247, p. 108-121, 1991Tradução . . Acesso em: 24 abr. 2024.
APA

Cayrel, R., Perrin, M. N., Barbuy, B. L. S., & Buser, R. (1991). Grid of synthetic spectra for the determination of effective temperature, gravity and metallicity of f, g, and k stars: I. Description of the method. Astronomy and Astrophysics, 247, 108-121.
NLM

Cayrel R, Perrin MN, Barbuy BLS, Buser R. Grid of synthetic spectra for the determination of effective temperature, gravity and metallicity of f, g, and k stars: I. Description of the method. Astronomy and Astrophysics. 1991 ; 247 108-121.[citado 2024 abr. 24 ]
Vancouver

Cayrel R, Perrin MN, Barbuy BLS, Buser R. Grid of synthetic spectra for the determination of effective temperature, gravity and metallicity of f, g, and k stars: I. Description of the method. Astronomy and Astrophysics. 1991 ; 247 108-121.[citado 2024 abr. 24 ]