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HI in Low-Luminosity Early-Type Galaxies | Tom Oosterloo
; Raffaella Morganti
; Elaine Sadler
; | Date: |
7 Sep 1998 | Subject: | astro-ph | Abstract: | 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. | Source: | arXiv, astro-ph/9809075 | Services: | Forum | Review | PDF | Favorites |
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