To use or not to use synthetic stellar spectra in population synthesis models? (2020)
- Authors:
- Autor USP: COELHO, PAULA RODRIGUES TEIXEIRA - IAG
- Unidade: IAG
- DOI: 10.1093/mnras/stz3609
- Subjects: GALÁXIAS; ATMOSFERAS ESTELARES
- Agências de fomento:
- Language: Inglês
- Imprenta:
- Source:
- Título: Monthly Notices of the Royal Astronomical Society
- Volume/Número/Paginação/Ano: v. 491, n.2, p.2025-2042, 2020
- Este periódico é de acesso aberto
- Este artigo NÃO é de acesso aberto
-
ABNT
COELHO, Paula Rodrigues Teixeira et al. To use or not to use synthetic stellar spectra in population synthesis models?. Monthly Notices of the Royal Astronomical Society, v. 491, n. 2, p. 2025-2042, 2020Tradução . . Disponível em: https://doi.org/10.1093/mnras/stz3609. Acesso em: 25 fev. 2026. -
APA
Coelho, P. R. T., Bruzual, G., Gonçalves, T. S., & Charlot, S. (2020). To use or not to use synthetic stellar spectra in population synthesis models? Monthly Notices of the Royal Astronomical Society, 491( 2), 2025-2042. doi:10.1093/mnras/stz3609 -
NLM
Coelho PRT, Bruzual G, Gonçalves TS, Charlot S. To use or not to use synthetic stellar spectra in population synthesis models? [Internet]. Monthly Notices of the Royal Astronomical Society. 2020 ; 491( 2): 2025-2042.[citado 2026 fev. 25 ] Available from: https://doi.org/10.1093/mnras/stz3609 -
Vancouver
Coelho PRT, Bruzual G, Gonçalves TS, Charlot S. To use or not to use synthetic stellar spectra in population synthesis models? [Internet]. Monthly Notices of the Royal Astronomical Society. 2020 ; 491( 2): 2025-2042.[citado 2026 fev. 25 ] Available from: https://doi.org/10.1093/mnras/stz3609 - Surface brightness fluctuation spectrum: a new probe of evolved stars inunresolved stellar populations
- Survival of molecular gas in a stellar feedback-driven outflow witnessed with the MUSE TIMER project and ALMA
- Stellar spectral models compared with empirical data
- The X-shooter spectral library (xsl): data release 2?,??
- Clocking the formation of today’s largest galaxies: wide field integral spectroscopy of brightest cluster galaxies and their surroundings
- A study on missing lines in the synthesic solar spectrum near the Ca triplet
- Spatial field reconstruction with INLA: application to IFU galaxy data
- Investigating the formation and evolution of massive disc galaxies with the MUSE TIMER project
- UV upturn versus UV weak galaxies: differences and similarities of their stellar populations unveiled by a de-biased sample
- Grids of synthetic spectra
Informações sobre o DOI: 10.1093/mnras/stz3609 (Fonte: oaDOI API)
How to cite
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
