Clocking the formation of today’s largest galaxies: wide field integral spectroscopy of brightest cluster galaxies and their surroundings (2020)
- Authors:
- Autor USP: COELHO, PAULA RODRIGUES TEIXEIRA - IAG
- Unidade: IAG
- DOI: 10.1093/mnras/stz2706
- Subjects: GALÁXIAS; POPULAÇÕES ESTELARES
- Agências de fomento:
- Language: Inglês
- Imprenta:
- Source:
- Título: Monthly Notices of the Royal Astronomical Society
- Volume/Número/Paginação/Ano: v. 491, n. 3, p. 2617-2638, 2020
- Este periódico é de acesso aberto
- Este artigo NÃO é de acesso aberto
-
ABNT
EDWARDS, Louise O. V e COELHO, Paula Rodrigues Teixeira. Clocking the formation of today’s largest galaxies: wide field integral spectroscopy of brightest cluster galaxies and their surroundings. Monthly Notices of the Royal Astronomical Society, v. 491, n. 3, p. 2617-2638, 2020Tradução . . Disponível em: https://doi.org/10.1093/mnras/stz2706. Acesso em: 14 fev. 2026. -
APA
Edwards, L. O. V., & Coelho, P. R. T. (2020). Clocking the formation of today’s largest galaxies: wide field integral spectroscopy of brightest cluster galaxies and their surroundings. Monthly Notices of the Royal Astronomical Society, 491( 3), 2617-2638. doi:10.1093/mnras/stz2706 -
NLM
Edwards LOV, Coelho PRT. Clocking the formation of today’s largest galaxies: wide field integral spectroscopy of brightest cluster galaxies and their surroundings [Internet]. Monthly Notices of the Royal Astronomical Society. 2020 ; 491( 3): 2617-2638.[citado 2026 fev. 14 ] Available from: https://doi.org/10.1093/mnras/stz2706 -
Vancouver
Edwards LOV, Coelho PRT. Clocking the formation of today’s largest galaxies: wide field integral spectroscopy of brightest cluster galaxies and their surroundings [Internet]. Monthly Notices of the Royal Astronomical Society. 2020 ; 491( 3): 2617-2638.[citado 2026 fev. 14 ] Available from: https://doi.org/10.1093/mnras/stz2706 - Surface brightness fluctuation spectrum: a new probe of evolved stars inunresolved stellar populations
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Informações sobre o DOI: 10.1093/mnras/stz2706 (Fonte: oaDOI API)
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