The stellar initial mass function of nearby young moving groups

Context. The solar neighbourhood is populated by nearby (<200 pc), young (<100 Myr) moving groups (NYMGs) of stars, whose origins are still a matter of debate. One plausible explanation is that they are remnants of individual stellar clusters and associations that are currently dispersing throughout...

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Detalles Bibliográficos

Principais autores:	Bertolotto-Stefanelli Rafael, José Downes Juan, Suárez Genaro, Mateu Cecilia, Gagné Jonathan, Román Zúñiga Carlos
Formato:	Artigo
Idioma:	Inglês
Publicado:	EDP Sciences 2026-02-01
Series:	Astronomy & Astrophysics
Assuntos:	open clusters and associations: general solar neighborhood galaxy: structure
Acceso en liña:	https://www.aanda.org/articles/aa/full_html/2026/02/aa57920-25/aa57920-25.html
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