An analysis of the composite stellar population in M32 (2010)
- Authors:
- Autor USP: OLIVEIRA, CLAUDIA LUCIA MENDES DE - IAG
- Unidade: IAG
- Subjects: GALÁXIAS; ESTRELAS; POPULAÇÕES ESTELARES
- Language: Inglês
- Imprenta:
- Publisher: Cambridge University Press
- Publisher place: Cambridge
- Date published: 2010
- Source:
- Conference titles: IAU Symposium
-
ABNT
COELHO, P e OLIVEIRA, Cláudia Lúcia Mendes de e FERNANDES, R. Cid. An analysis of the composite stellar population in M32. 2010, Anais.. Cambridge: Cambridge University Press, 2010. . Acesso em: 14 mar. 2026. -
APA
Coelho, P., Oliveira, C. L. M. de, & Fernandes, R. C. (2010). An analysis of the composite stellar population in M32. In Stellar populations : planning for the next decade. Proceedings. Cambridge: Cambridge University Press. -
NLM
Coelho P, Oliveira CLM de, Fernandes RC. An analysis of the composite stellar population in M32. Stellar populations : planning for the next decade. Proceedings. 2010 ;[citado 2026 mar. 14 ] -
Vancouver
Coelho P, Oliveira CLM de, Fernandes RC. An analysis of the composite stellar population in M32. Stellar populations : planning for the next decade. Proceedings. 2010 ;[citado 2026 mar. 14 ] - The Hα kinematics of interacting galaxies in 12 compact groups
- Two formation channels of ultra-compact dwarf galaxies in Hickson compact groups
- First results from SAM-FP: Fabry–Perot observations with ground-layer adaptive optics – the structure and kinematics of the core of 30 Doradus
- Rotation curve bifurcations as indicators of close recent galaxy encounters
- The Tully–Fisher relations for Hickson compact group galaxies
- Star-forming regions and the metallicity gradients in the tidal tails: the case of NGC 92
- Searching for planetary nebulae at the Galactic halo via J-PAS
- Tidal dwarf galaxies in the stephan's quintet?
- The Hydra I cluster core: II. Kinematic complexity in a rising velocity dispersion profile around the cD galaxy NGC 3311
- Kinematics of the outskirts of S0 galaxies from PNe and GCs
How to cite
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
