The Hamburg/ESO R-process enhanced star survey (HERES): II. Spectroscopic analysis of the survey sample (2005)
- Authors:
- Autor USP: ROSSI, SILVIA CRISTINA FERNANDES - IAG
- Unidade: IAG
- Subjects: GALÁXIAS; ASTROFÍSICA ESTELAR
- Language: Inglês
- Imprenta:
- Source:
- Título do periódico: Astronomy and Astrophysics
- ISSN: 0004-6361
- Volume/Número/Paginação/Ano: V. 439, p. 129-151, 2005
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ABNT
BARKLEM, P.S et al. The Hamburg/ESO R-process enhanced star survey (HERES): II. Spectroscopic analysis of the survey sample. Astronomy and Astrophysics, p. 129-151, 2005Tradução . . Acesso em: 30 abr. 2024. -
APA
Barklem, P. S., Chistlieb, N., Beers, T. C., Hill, V., Bessell, M. S., Holmberg, J., et al. (2005). The Hamburg/ESO R-process enhanced star survey (HERES): II. Spectroscopic analysis of the survey sample. Astronomy and Astrophysics, 129-151. -
NLM
Barklem PS, Chistlieb N, Beers TC, Hill V, Bessell MS, Holmberg J, Marsteller B, Rossi SCF, Zickgraf F-J, Reimers D. The Hamburg/ESO R-process enhanced star survey (HERES): II. Spectroscopic analysis of the survey sample. Astronomy and Astrophysics. 2005 ; 129-151.[citado 2024 abr. 30 ] -
Vancouver
Barklem PS, Chistlieb N, Beers TC, Hill V, Bessell MS, Holmberg J, Marsteller B, Rossi SCF, Zickgraf F-J, Reimers D. The Hamburg/ESO R-process enhanced star survey (HERES): II. Spectroscopic analysis of the survey sample. Astronomy and Astrophysics. 2005 ; 129-151.[citado 2024 abr. 30 ] - 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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