Determination of kinematic distances of pre main sequence stars in star-forming regions (2010)
- Authors:
- Autor USP: TEIXEIRA, RAMACHRISNA - IAG
- Unidade: IAG
- Subjects: DISTÂNCIAS ESTELARES; CINEMÁTICA; EVOLUÇÃO ESTELAR; FORMAÇÃO DE ESTRELAS
- Language: Inglês
- Imprenta:
- Publisher: Cambridge University Press
- Publisher place: Cambridge
- Date published: 2010
- Source:
- Conference titles: IAU Symposium
-
ABNT
GALLI, Phillip A. B et al. Determination of kinematic distances of pre main sequence stars in star-forming regions. 2010, Anais.. Cambridge: Cambridge University Press, 2010. . Acesso em: 24 jan. 2026. -
APA
Galli, P. A. B., Ducourant, C., Bertout, C., & Teixeira, R. (2010). Determination of kinematic distances of pre main sequence stars in star-forming regions. In Stars clusters : basic galactic building throughout time and space. Proceedings. Cambridge: Cambridge University Press. -
NLM
Galli PAB, Ducourant C, Bertout C, Teixeira R. Determination of kinematic distances of pre main sequence stars in star-forming regions. Stars clusters : basic galactic building throughout time and space. Proceedings. 2010 ;[citado 2026 jan. 24 ] -
Vancouver
Galli PAB, Ducourant C, Bertout C, Teixeira R. Determination of kinematic distances of pre main sequence stars in star-forming regions. Stars clusters : basic galactic building throughout time and space. Proceedings. 2010 ;[citado 2026 jan. 24 ] - A kinematic study and membership analysis of the Lupus star-forming region
- Full sky survey for common proper motion stars
- Kinematic distances of pre-main-sequence stars in the Lupus star-forming region
- IPERCOOL - an international program for the study of sub-stellar objects
- kinematic distances of pre-main sequence stars in nearby star-forming regions
- Origin of the wide-orbit circumbinary giant planet HD-106906 - A dynamical scenario and its impact on the disk
- A new method for calculating the convergent point of a moving group
- Movimento próprio de estrelas pré-sequência principal
- Vendo o invisível na missão ESA-Gaia: objetos fracos e análise de galáxias não resolvidas
- Estrelas fracas nas vizinhanças solares
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