HI in Early-Type Galaxies

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dc.creatorOosterloo, T.
dc.creatorMorganti, R.
dc.creatorSadler, E. M.
dc.date2000-09-07
dc.date.accessioned2026-07-07T01:55:22Z
dc.date.available2026-07-07T01:55:22Z
dc.descriptionWe briefly discuss the main differences between the HI properties of luminous and low-luminosity early-type galaxies. In luminous early-type galaxies the HI is often irregularly distributed, but in a few cases regular HI disks, of low surface density, are seen. In low-luminosity galaxies, the HI is more often in a disk with high central surface densities. This suggests a different evolution of the gas in these two groups of galaxies.
dc.descriptionTo appear in the proceedings of the conference "Gas and Galaxy Evolution" (ASP Conference Series), eds. J. Hibbard, M. Rupen, and J. van Gorkom
dc.identifierhttps://arxiv.org/abs/astro-ph/0009112
dc.identifierhttp://arxiv.org/abs/astro-ph/0009112
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1631
dc.subjectAstrophysics
dc.titleHI in Early-Type Galaxies
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