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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Guardado en:
Detalles Bibliográficos
Publicado: 1998
Materias:
Galaxies: dwarf
Galaxies: formation
Galaxies: individual: NGC 5291
Galaxies: interactions
Galaxies: ISM
Radio lines: galaxies
Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046361_v333_n3_p813_Duc
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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