Large-scale HI structures and the origin of radio galaxies

R Morganti*, T Oosterloo, C Tadhunter, B Emonts

*Bijbehorende auteur voor dit werk

OnderzoeksoutputAcademicpeer review

3 Citaten (Scopus)
218 Downloads (Pure)

Samenvatting

We present the first results of a study aimed to detect large H I structures in radio galaxies. In two of the three cases presented (Coma A and B2 0648 + 27), the detection of a large amount of H I distributed over several tens of kpc suggests a major merger as the origin of the observed system and allows us to infer when this merger must have occurred. The situation is less clear for the third object (3C 433). We propose an evolutionary sequence for one of the radio galaxies studied. The implications of this study of neutral hydrogen in nearby radio galaxies for high-z objects and 'normal' (i.e. radio-quiet) elliptical galaxies are also discussed. (C) 2003 Elsevier B.V. All rights reserved.

Originele taal-2English
Pagina's (van-tot)273-277
Aantal pagina's5
TijdschriftNew Astronomy Reviews
Volume47
Nummer van het tijdschrift4-5
DOI's
StatusPublished - sep-2003
EvenementWorkshop on High-Redshift Radio Galaxies - Past Present and future - , Netherlands
Duur: 11-nov-200215-nov-2002

Citeer dit