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Spatially resolved stellar populations and emission line properties in nearby galaxies with J-PLUS

Aims. We aim to characterize the spatially resolved stellar population and emission-line properties of galaxies in the M51 group using the same methodology previously applied to the M101 group, ultimately seeking to understand how environmental processes shape the physical properties of galaxies by...

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Tallennettuna:
Päätekijät: Thainá-Batista J., Cid Fernandes R., González Delgado R. M., Rodríguez-Martín J. E., García-Benito R., Díaz-García L. A., Martínez-Solaeche G., Ruschel-Dutra D., Sasse V. H., Cenarro A. J., Cristóbal-Hornillos D., Hernández-Monteagudo C., López-Sanjuan C., Marín-Franch A., Moles M., Varela J., Vázquez Ramió H., Alcaniz J., Dupke R. A., Ederoclite A., Sodré L., Angulo R. E.
Aineistotyyppi: Artigo
Kieli:Inglês
Julkaistu: EDP Sciences 2026-04-01
Sarja:Astronomy & Astrophysics
Aiheet:
methods: data analysis
techniques: photometric
astronomical databases: miscellaneous
galaxies: general
galaxies: individual: m51
galaxies: individual: m63
galaxies: stellar content
Linkit:https://www.aanda.org/articles/aa/full_html/2026/04/aa57271-25/aa57271-25.html
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