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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Principais autores:	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.
פורמט:	Artigo
שפה:	Inglês
יצא לאור:	EDP Sciences 2026-04-01
סדרה:	Astronomy & Astrophysics
נושאים:	methods: data analysis techniques: photometric astronomical databases: miscellaneous galaxies: general galaxies: individual: m51 galaxies: individual: m63 galaxies: stellar content
גישה מקוונת:	https://www.aanda.org/articles/aa/full_html/2026/04/aa57271-25/aa57271-25.html
תגים:	הוספת תג אין תגיות, היה/י הראשונ/ה לתייג את הרשומה!