Self-consistent physical parameters for mC clusters from CMD modelling: application to SMC clusters observed with the soar telescope (2008)
- Authors:
- Autor USP: BARBUY, BEATRIZ LEONOR SILVEIRA - IAG
- Unidade: IAG
- Assunto: GALÁXIA
- Language: Inglês
- Imprenta:
- Source:
- Título: Boletim da Sociedade Astronômica Brasileira
- ISSN: 0101-3440
- Volume/Número/Paginação/Ano: v. 28, n. 1, p. 224, 2008
- Conference titles: Reunião Anual da Sociedade astronômica Brasileira
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ABNT
DIAS, Bruno et al. Self-consistent physical parameters for mC clusters from CMD modelling: application to SMC clusters observed with the soar telescope. Boletim da Sociedade Astronômica Brasileira. São Paulo: Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo. . Acesso em: 09 jan. 2026. , 2008 -
APA
Dias, B., Kerber, L., Barbuy, B. L. S., & Santiago, B. (2008). Self-consistent physical parameters for mC clusters from CMD modelling: application to SMC clusters observed with the soar telescope. Boletim da Sociedade Astronômica Brasileira. São Paulo: Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo. -
NLM
Dias B, Kerber L, Barbuy BLS, Santiago B. Self-consistent physical parameters for mC clusters from CMD modelling: application to SMC clusters observed with the soar telescope. Boletim da Sociedade Astronômica Brasileira. 2008 ; 28( 1): 224.[citado 2026 jan. 09 ] -
Vancouver
Dias B, Kerber L, Barbuy BLS, Santiago B. Self-consistent physical parameters for mC clusters from CMD modelling: application to SMC clusters observed with the soar telescope. Boletim da Sociedade Astronômica Brasileira. 2008 ; 28( 1): 224.[citado 2026 jan. 09 ] - MOSAIC at the E-ELT: a multi-object spectrograph for Astrophysics, IGM and Cosmology
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