Mapping the galaxy NGC 4486 (M87) through its globular cluster system

As shown in previous works, globular clusters (GCs) can be used to trace the overall structure of the diffuse stellar populations in early-type galaxies if the number of clusters per unit stellar mass depends on metallicity. In this paper we further test this assumption in the galaxy NGC 4486 (M87)...

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Detalles Bibliográficos
Autores principales:	Forte, Juan Carlos, Vega, Ema Irene, Faifer, Favio Raúl
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2012
Materias:	Ciencias Astronómicas Galaxies: haloes Galaxies: star clusters: general Globular clusters: general
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/84681
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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