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HI in Early-Type Galaxies | | T. Oosterloo
; R. Morganti
; E.M. Sadler
; | | Date: |
7 Sep 2000 | | Subject: | astro-ph | | Affiliation: | NFRA), R. Morganti (NFRA), E.M. Sadler (Sydney | | Abstract: | We 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. | | Source: | arXiv, astro-ph/0009112 | | Other source: | [GID 36000] astro-ph/9902011 | | Services: | Forum | Review | PDF | Favorites | |
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