| | |
| | |
Stat |
Members: 3645 Articles: 2'504'585 Articles rated: 2609
24 April 2024 |
|
| | | |
|
Article overview
| |
|
Lenticular galaxies at the outskirts of the Leo II group: NGC 3599 and NGC 3626 | O. K. Sil'chenko
; A. V. Moiseev
; A. P. Shulga
; | Date: |
13 Oct 2010 | Abstract: | We have studied unbarred S0 galaxies, NGC 3599 and NGC 3626, the members of
the X-ray bright group Leo II, by means of 3D spectroscopy, long-slit
spectroscopy, and imaging, with the aim to identify epoch and mechanismsof
their transformation from spirals. Both galaxies have appeared to bear a
complex of features resulting obviously from minor merging: decoupled gas
kinematics, nuclear starforming rings, and multi-tiered oval large-scale
stellar disks. The weak-emission line nucleus of NGC 3599 bears all signs of
the Seyfert activity, according to the line-ratio diagnostics of the gas
excitation mechanism. After all, we conclude that the transformation of these
lenticular galaxies has had place about 1-2 Gyr ago, through the gravitational
mechanisms not related to hot intragroup medium of Leo II. | Source: | arXiv, 1010.2716 | Services: | Forum | Review | PDF | Favorites |
|
|
No review found.
Did you like this article?
Note: answers to reviews or questions about the article must be posted in the forum section.
Authors are not allowed to review their own article. They can use the forum section.
browser Mozilla/5.0 AppleWebKit/537.36 (KHTML, like Gecko; compatible; ClaudeBot/1.0; +claudebot@anthropic.com)
|
| |
|
|
|
| News, job offers and information for researchers and scientists:
| |