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03 December 2021
 
  » arxiv » astro-ph/0009112

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HI in Early-Type Galaxies
T. Oosterloo ; R. Morganti ; E.M. Sadler ;
Date 7 Sep 2000
Subject astro-ph
AffiliationNFRA), R. Morganti (NFRA), E.M. Sadler (Sydney
AbstractWe 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
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