Morphology of galaxies with quiescent recent assembly history in a Λ-CDM universe

Context. The standard disc formation scenario postulates that the disc forms as the gas cools and flows into the centre of the dark matter halo, conserving the specific angular momentum. Major mergers have been shown to be able to destroy or highly perturb the disc components. More recently, the ali...

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Detalles Bibliográficos
Autores principales:	Pedrosa, S.E., Tissera, P.B., De Rossi, M.E.
Formato:	JOUR
Materias:	Galaxies: evolution Galaxies: formation Galaxies: structure Angular momentum Mergers and acquisitions Merging Morphology Supernovae Angular momentum orientation Complex Processes Dark matter halos Galaxies: evolutions Galaxy formations Hier-archical clustering Galaxies
Acceso en línea:	http://hdl.handle.net/20.500.12110/paper_00046361_v567_n_p_Pedrosa
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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