Estimation of stellar metal abundance. II. A recalibration of the 'CA' II 'K' technique, and autocorrelation function method (1999)
- Authors:
- Autor USP: ROSSI, SILVIA CRISTINA FERNANDES - IAG
- Unidade: IAG
- Subjects: ASTRONOMIA; GALÁXIAS
- Language: Inglês
- Imprenta:
- Source:
- Título: Astronomical Journal
- Volume/Número/Paginação/Ano: v. 117, n. 2, p. 981-1009, Feb. 1999
-
ABNT
BEERS, Timothy C. et al. Estimation of stellar metal abundance. II. A recalibration of the 'CA' II 'K' technique, and autocorrelation function method. Astronomical Journal, v. 117, n. 2, p. 981-1009, 1999Tradução . . Acesso em: 14 jul. 2025. -
APA
Beers, T. C., Rossi, S. C. F., Norris, J. E., Ryan, S. G., & Shefler, T. (1999). Estimation of stellar metal abundance. II. A recalibration of the 'CA' II 'K' technique, and autocorrelation function method. Astronomical Journal, 117( 2), 981-1009. -
NLM
Beers TC, Rossi SCF, Norris JE, Ryan SG, Shefler T. Estimation of stellar metal abundance. II. A recalibration of the 'CA' II 'K' technique, and autocorrelation function method. Astronomical Journal. 1999 ; 117( 2): 981-1009.[citado 2025 jul. 14 ] -
Vancouver
Beers TC, Rossi SCF, Norris JE, Ryan SG, Shefler T. Estimation of stellar metal abundance. II. A recalibration of the 'CA' II 'K' technique, and autocorrelation function method. Astronomical Journal. 1999 ; 117( 2): 981-1009.[citado 2025 jul. 14 ] - Descoberta e análise de objetos com linhas em emissão no Survey HK
- A search for unrecognized carbon-enchanced metal-poor stars
- s/r ratios in carbon-enhanced metal-poor stars
- Stellar spectra
- A continued search for CEMP RR Lyrae stars
- Searching for s-process-enhanced metal-poor stars
- Estimation of carbon abundances in metal-poor stars. I. application to the strong g-band stars of beers, preston, and shectman
- The stellar content of the Hamburg/ESO survey: III. field horizontal-branch stars in the galaxy
- The ideal stars for exploration of early-epoch 'ANTIPOT.7 LI' abundances
- Spectroscopic validation of low-metallicity stars from RAVE
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