Evidence for gas accretion in galactic disks

dc.creatorvan der Hulst, Thijs
dc.creatorSancisi, Renzo
dc.date2003-12-24
dc.date.accessioned2026-07-07T02:11:44Z
dc.date.available2026-07-07T02:11:44Z
dc.descriptionStudies of the HI in galaxies have clearly shown that subtle details of the HI distribution and kinematics often harbour key information for understanding the structure and evolution of galaxies. Evidence for the accretion of material has grown over the past many years and clear signatures can be found in HI observations of galaxies. We have obtained new detailed and sensitive HI synthesis observations of three nearby galaxies which are suspected of capturing small amounts of HI and show that indeed accretion of small amounts of gas is taking place in these galaxies. This could be the same kind of phenomenon of material infall as observed in the stellar streams in the halo and outer parts of our galaxy and M31
dc.descriptionTo appear in the proceedings of the IAU Symposium #217, Recycling Intergalactic and Interstellar Matter, eds. P.-A. Duc, J. Braine, and E. Brinks, 8 pages
dc.identifierhttps://arxiv.org/abs/astro-ph/0312613
dc.identifierhttp://arxiv.org/abs/astro-ph/0312613
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/7203
dc.subjectAstrophysics
dc.titleEvidence for gas accretion in galactic disks
dc.typetext

Files

Collections