UV upturn versus UV weak galaxies: differences and similarities of their stellar populations unveiled by a de-biased sample (2020)
- Authors:
- Autor USP: COELHO, PAULA RODRIGUES TEIXEIRA - IAG
- Unidade: IAG
- DOI: 10.1093/mnras/staa3447
- Subjects: COSMOLOGIA; AGLOMERADOS DE GALÁXIAS; UNIVERSO PRIMORDIAL
- Agências de fomento:
- Language: Inglês
- Imprenta:
- Source:
- Título: Monthly Notices of the Royal Astronomical Society
- ISSN: 1365-2966
- Volume/Número/Paginação/Ano: h v. 500, n. 2, p. 1870–1883, 2020
- Este periódico é de acesso aberto
- Este artigo NÃO é de acesso aberto
-
ABNT
DANTAS, M L L e COELHO, Paula R. T. e SÁNCHEZ-BLÁSQUEZ, P. UV upturn versus UV weak galaxies: differences and similarities of their stellar populations unveiled by a de-biased sample. Monthly Notices of the Royal Astronomical Society, v. h 500, n. 2, p. 1870–1883, 2020Tradução . . Disponível em: https://doi.org/10.1093/mnras/staa3447. Acesso em: 20 jan. 2026. -
APA
Dantas, M. L. L., Coelho, P. R. T., & Sánchez-Blásquez, P. (2020). UV upturn versus UV weak galaxies: differences and similarities of their stellar populations unveiled by a de-biased sample. Monthly Notices of the Royal Astronomical Society, h 500( 2), 1870–1883. doi:10.1093/mnras/staa3447 -
NLM
Dantas MLL, Coelho PRT, Sánchez-Blásquez P. UV upturn versus UV weak galaxies: differences and similarities of their stellar populations unveiled by a de-biased sample [Internet]. Monthly Notices of the Royal Astronomical Society. 2020 ;h 500( 2): 1870–1883.[citado 2026 jan. 20 ] Available from: https://doi.org/10.1093/mnras/staa3447 -
Vancouver
Dantas MLL, Coelho PRT, Sánchez-Blásquez P. UV upturn versus UV weak galaxies: differences and similarities of their stellar populations unveiled by a de-biased sample [Internet]. Monthly Notices of the Royal Astronomical Society. 2020 ;h 500( 2): 1870–1883.[citado 2026 jan. 20 ] Available from: https://doi.org/10.1093/mnras/staa3447 - A new library of theoretical stellar spectra for stellar population applications
- Inside-out formation of nuclear discs and the absence of old central spheroids in barred galaxies of the TIMER survey
- Grids of synthetic spectra
- High-resolution spectral line indices useful for the analysis of stellar populations
- Biblioteca de espectros sintéticos de alta resolução, do ultravioleta ao infravermelho, com razão ['ALFA'/ Fe] variável, para síntese de populações estelares
- Spatial field reconstruction with INLA: application to IFU galaxy data
- Investigating the formation and evolution of massive disc galaxies with the MUSE TIMER project
- Self-similarity in the chemical evolution of galaxies and the delay-time distribution of SNe Ia
- The fossil record of the stellar populations at redshifts above 1.5
- Central enhancement of the nitrogen-to-oxygen abundance ratio in barred galaxies
Informações sobre o DOI: 10.1093/mnras/staa3447 (Fonte: oaDOI API)
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