Young tidal dwarf galaxies around the gas-rich disturbed lenticular NGC 5291

NGC 5291 is an early type galaxy at the edge of the cluster Abell 3574 which drew the attention because of the unusual high amount of atomic gas (∼ 5 × 10110 M·) found associated to it. The HI is distributed along a huge and fragmented ring, possibly formed after a tidal interaction with a companion...

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Detalles Bibliográficos
Autores principales:	Duc, P.-A., Mirabel, I.F.
Formato:	JOUR
Materias:	Galaxies: dwarf Galaxies: formation Galaxies: individual: NGC 5291 Galaxies: interactions Galaxies: ISM Radio lines: galaxies
Acceso en línea:	http://hdl.handle.net/20.500.12110/paper_00046361_v333_n3_p813_Duc
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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