Mapeamento Ambiental de Galáxias Pós-Starburst
DOI:
https://doi.org/10.47456/Cad.Astro.v7nEspecial.53386Palavras-chave:
galáxias pós-starburst, quenching, ambiente de galáxiasResumo
Resumo do pôster apresentado na terceira edição do evento As Astrocientistas, realizado entre os dias 31 de março e 4 de abril de 2025.
Referências
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[4] S. Alam, F. D. Albareti, C. A. Prieto, F. Anders, S. F. Anderson, T. Anderton, B. H. Andrews, E. Armengaud, É. Aubourg, S. Bailey et al., The eleventh and twelfth data releases of the sloan digital sky survey: final data from sdss-iii, The Astrophysical Journal Supplement Series 219 (1), 12 (2015).
[5] S. Salim, J. C. Lee, S. Janowiecki, E. d. Cunha, M. Dickinson, M. Boquien, D. Burgarella, J. J. Salzer e S. Charlot, Galex–sdss– wise legacy catalog (gswlc): Star formation rates, stellar masses, and dust attenuations of 700,000 low-redshift galaxies, The Astrophysical Journal Supplement Series 227 (1), 2 (2016).
[6] H. M. Yesuf, Quenching in the right place at the right time: Tracing the shared history of starbursts, active galactic nuclei, and poststarburst galaxies using their structures and multiscale environments, The Astrophysical Journal 936 (2), 124 (2022).
[7] E. Tempel, T. Tuvikene, R. Kipper e N. I. Libeskind, Merging groups and clusters of galaxies from the sdss data-the catalogue of groups and potentially merging systems, Astronomy & Astrophysics 602, A100 (2017).
[8] R. C. Kennicutt Jr, Star formation in galaxies along the hubble sequence, Annual Review of Astronomy and Astrophysics 36 (1), 189 (1998).
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Direitos autorais (c) 2026 Rafaela Conz da Costa, Sandro Barboza Rembold

Este trabalho está licenciado sob uma licença Creative Commons Attribution 4.0 International License.



