HI in Low-Luminosity Early-Type Galaxies

Details HI in Low-Luminosity Early-Type Galaxies HI in Low-Luminosity Early-Type Galaxies

1998-09-07

arxiv.org/abs/astro-ph/9809075v1

Astronomy and Astrophysics

Astrophysics

to appear in Star Formation in Early-Type Galaxies, ASP Conf. Ser., eds. P. Carral & J. Cepa; 10 pages, 11 figures, paspconf.s

Scientific paper

We 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.

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