Spectroscopy of hot stars in the galactic halo. III. analysis of a large sample of field horizontal-branch and other a-type stars (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. 5, p. 2329-2380, May 1999
-
ABNT
WILHELM, Ronald et al. Spectroscopy of hot stars in the galactic halo. III. analysis of a large sample of field horizontal-branch and other a-type stars. Astronomical Journal, v. 117, n. 5, p. 2329-2380, 1999Tradução . . Acesso em: 04 mar. 2026. -
APA
Wilhelm, R., Beers, T. C., Sommer-Larsen, J., Pier, J. R., Layden, A. C., Flynn, C., et al. (1999). Spectroscopy of hot stars in the galactic halo. III. analysis of a large sample of field horizontal-branch and other a-type stars. Astronomical Journal, 117( 5), 2329-2380. -
NLM
Wilhelm R, Beers TC, Sommer-Larsen J, Pier JR, Layden AC, Flynn C, Rossi SCF, Christensen PR. Spectroscopy of hot stars in the galactic halo. III. analysis of a large sample of field horizontal-branch and other a-type stars. Astronomical Journal. 1999 ; 117( 5): 2329-2380.[citado 2026 mar. 04 ] -
Vancouver
Wilhelm R, Beers TC, Sommer-Larsen J, Pier JR, Layden AC, Flynn C, Rossi SCF, Christensen PR. Spectroscopy of hot stars in the galactic halo. III. analysis of a large sample of field horizontal-branch and other a-type stars. Astronomical Journal. 1999 ; 117( 5): 2329-2380.[citado 2026 mar. 04 ] - Broadband UBVRcIc photometry of horizontal-branch and metal-poor candidates from the HK and Hamburg/ESO surveys. I.
- Metal-poor stars observed with the Magellan Telescope.: II. Discovery of four stars with [Fe/H] <= -3,5
- The Hamburg/ESO R-process enhanced star survey (HERES): II. Spectroscopic analysis of the survey sample
- Metal abundance estimates for F- and G-type stars from Edinburgh-cape blue object survey
- Estimativas de precisão de temperaturas efetivas estelares e avermelhamento interestelar utilizando o índice de linha de Balmer baseado em espectroscopia de média resolução
- Bright metal-poor stars from the Hamburg/ESO survey: I. Selection and follow-up observations from 329 fields
- The R-Process Alliance: Spectroscopic Follow-up of Low-metallicity Star Candidates from the Best & Brightest Survey
- Elemental abundances and classification of carbon-enhanced metal-poor stars
- Additional emission-line candidates from the hk survey
- Spectroscopic validation of low-metallicity stars from RAVE
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