The potential of JPAS and APLUS for the study of small stellar systems (2015)
- Authors:
- USP affiliated authors: OLIVEIRA, CLAUDIA LUCIA MENDES DE - IAG ; COELHO, PAULA RODRIGUES TEIXEIRA - IAG
- Unidade: IAG
- Subjects: ESTRELAS; POPULAÇÕES ESTELARES; INSTRUMENTAÇÃO (ASTRONOMIA)
- Language: Inglês
- Imprenta:
- Publisher: International Astronomical Union
- Publisher place: Paris
- Date published: 2015
- Source:
- Título do periódico: Meeting Abstracts
- Conference titles: IAU General Assembly
-
ABNT
SANTOS, A. Chies et al. The potential of JPAS and APLUS for the study of small stellar systems. 2015, Anais.. Paris: International Astronomical Union, 2015. . Acesso em: 19 abr. 2024. -
APA
Santos, A. C., Oliveira, C. L. M. de, Cenarro, J., Cortesi, A., & Coelho, P. R. T. (2015). The potential of JPAS and APLUS for the study of small stellar systems. In Meeting Abstracts. Paris: International Astronomical Union. -
NLM
Santos AC, Oliveira CLM de, Cenarro J, Cortesi A, Coelho PRT. The potential of JPAS and APLUS for the study of small stellar systems. Meeting Abstracts. 2015 ;[citado 2024 abr. 19 ] -
Vancouver
Santos AC, Oliveira CLM de, Cenarro J, Cortesi A, Coelho PRT. The potential of JPAS and APLUS for the study of small stellar systems. Meeting Abstracts. 2015 ;[citado 2024 abr. 19 ] - One hundred SMUDGes in S-PLUS: ultra-diffuse galaxies flourish in the field
- J-PLUS: the impact of bars on quenching time-scales in nearby green valley disc galaxies
- J-PLUS: measuring Hα emission line fluxes in the nearby universe
- J-PLUS: Two-dimensional analysis of the stellar population in NGC 5473 and NGC 5485
- A new library of theoretical stellar spectra for stellar population applications
- Self-similarity in the chemical evolution of galaxies and the delay-time distribution of SNe Ia
- Surface brightness fluctuation spectrum: a new probe of evolved stars inunresolved stellar populations
- UV upturn versus UV weak galaxies: differences and similarities of their stellar populations unveiled by a de-biased sample
- Clocking the formation of today’s largest galaxies: wide field integral spectroscopy of brightest cluster galaxies and their surroundings
- To use or not to use synthetic stellar spectra in population synthesis models?
How to cite
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
