The mass-metallicity relation of interacting galaxies

We study the mass-metallicity relation of galaxies in pairs and in isolation taken from the Sloan Digital Sky Survey-Data Release 4 (SDSS-DR4) using the stellar masses and oxygen abundances derived by Tremonti et al. Close galaxy pairs, defined by projected separation rp < 25 kpc h-1 and radi...

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Detalles Bibliográficos
Autores principales:	Michel-Dansac, L., Lambas, D.G., Alonso, M.S., Tissera, P.
Formato:	JOUR
Materias:	Galaxies: abundances Galaxies: evolution Galaxies: formation Galaxies: interactions
Acceso en línea:	http://hdl.handle.net/20.500.12110/paper_17453933_v386_n1_pL82_MichelDansac
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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