|
| | | | |
| | | |
| Stat |
Members: 3645
Articles: 2'500'096
Articles rated: 2609
19 April 2024 |
|
| | | | |
|
Article forum
| |
|
|
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 | |
|
|
No message found in this article forum.
You have a question or message about this article?
Ask the community and write a message in the forum.
If you want to rate this article, please use the review section..
To add a message in the forum, you need to login or register first. (free): registration page
|
| |
|
|
|
|
News, job offers and information for researchers and scientists:
| |
REGISTER