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
- Status:
- Artigo possui versão em acesso aberto em repositório (Green Open Access)
- Versão do Documento:
- Versão aceita (Póst-print)
- Acessar versão aberta:
-
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: 06 maio 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 maio 06 ] 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 maio 06 ] Available from: https://doi.org/10.1093/mnras/staa3447 - Surface brightness fluctuation spectrum: a new probe of evolved stars inunresolved stellar populations
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