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:
- 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 ] - Gente do céu
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- Stellar populations in elliptical galaxies of compact groups
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