A spectroscopic survey of FHB stars near the south galactic pole (2010)
- Authors:
- USP affiliated authors: COSTA, ROBERTO DELL'AGLIO DIAS DA - IAG ; ROSSI, SILVIA CRISTINA FERNANDES - IAG
- Unidade: IAG
- Subjects: ESTRELAS; ESPECTROSCOPIA; ASTROFÍSICA ESTELAR
- Language: Inglês
- Imprenta:
- Publisher: Cambridge University Press
- Publisher place: Cambridge
- Date published: 2010
- Source:
- Conference titles: IAU Symposium
-
ABNT
ROSSI, Silvia Cristina Fernandes et al. A spectroscopic survey of FHB stars near the south galactic pole. 2010, Anais.. Cambridge: Cambridge University Press, 2010. . Acesso em: 28 jan. 2026. -
APA
Rossi, S. C. F., Ortiz, R., Wilhelm, R., Costa, R. D. 'A. D. da, & Beers, T. C. (2010). A spectroscopic survey of FHB stars near the south galactic pole. In Stellar populations : planning for the next decade. Proceedings. Cambridge: Cambridge University Press. -
NLM
Rossi SCF, Ortiz R, Wilhelm R, Costa RD'AD da, Beers TC. A spectroscopic survey of FHB stars near the south galactic pole. Stellar populations : planning for the next decade. Proceedings. 2010 ;[citado 2026 jan. 28 ] -
Vancouver
Rossi SCF, Ortiz R, Wilhelm R, Costa RD'AD da, Beers TC. A spectroscopic survey of FHB stars near the south galactic pole. Stellar populations : planning for the next decade. Proceedings. 2010 ;[citado 2026 jan. 28 ] - Diagnóstico dos objetos encontrados no survey espectroscópio na direção do pólo sul galáctico
- A search for field horizontal-branch stars near the south galactic pole
- A survey of Early-Type Stars based on the two micron all sky survey database
- Additional emission-line candidates from the hk survey
- Spectroscopic validation of low-metallicity stars from RAVE
- High-resolution spectroscopy of giant stars in the open clusters IC 4651 and IC 4725
- Identification and analysis of horizontal-branch and other A-type stars in the galaxy
- The age structure of the Milky Way’s halo
- Descoberta e análise de objetos com linhas em emissão no survey HK
- Searching for chemical classes among metal-poor stars using medium-resolution spectroscopy
How to cite
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
