The frequency of warm carbon-enhanced metal-poor stars in SDSS-I DR-5 (2007)
- Authors:
- Autor USP: ROSSI, SILVIA CRISTINA FERNANDES - IAG
- Unidade: IAG
- Subjects: ESTRELAS; METAIS; ASTROQUÍMICA
- Language: Inglês
- Imprenta:
- Publisher place: Washington
- Date published: 2007
- Conference titles: 2007 AAS/AAPT Joint Meeting
-
ABNT
MARSTELLER, Brian E et al. The frequency of warm carbon-enhanced metal-poor stars in SDSS-I DR-5. 2007, Anais.. Washington: Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo, 2007. . Acesso em: 25 abr. 2024. -
APA
Marsteller, B. E., Beers, T. C., Sivarani, T., Rossi, S. C. F., Knapp, J., Plez, B., et al. (2007). The frequency of warm carbon-enhanced metal-poor stars in SDSS-I DR-5. In . Washington: Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo. -
NLM
Marsteller BE, Beers TC, Sivarani T, Rossi SCF, Knapp J, Plez B, Johnson J, Masseron T. The frequency of warm carbon-enhanced metal-poor stars in SDSS-I DR-5. 2007 ;[citado 2024 abr. 25 ] -
Vancouver
Marsteller BE, Beers TC, Sivarani T, Rossi SCF, Knapp J, Plez B, Johnson J, Masseron T. The frequency of warm carbon-enhanced metal-poor stars in SDSS-I DR-5. 2007 ;[citado 2024 abr. 25 ] - 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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