HI in Low-Luminosity Early-Type Galaxies

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dc.creatorOosterloo, Tom
dc.creatorMorganti, Raffaella
dc.creatorSadler, Elaine
dc.date1998-09-07
dc.date.accessioned2026-07-07T02:27:50Z
dc.date.available2026-07-07T02:27:50Z
dc.descriptionWe discuss the properties of the HI in low-luminosity early-type galaxies. The morphology of the HI is more regular than that of the HI in many more-luminous early-type galaxies. The HI is always distributed in a disk and is more centrally concentrated. The central HI surface densities are higher than in luminous early-type galaxies and are high enough for star formation to occur.
dc.descriptionto appear in Star Formation in Early-Type Galaxies, ASP Conf. Ser., eds. P. Carral & J. Cepa; 10 pages, 11 figures, paspconf.sty LateX
dc.identifierhttps://arxiv.org/abs/astro-ph/9809075
dc.identifierhttp://arxiv.org/abs/astro-ph/9809075
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/12864
dc.subjectAstrophysics
dc.titleHI in Low-Luminosity Early-Type Galaxies
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