|
| | | | |
| | | |
| Stat |
Members: 3645
Articles: 2'503'724
Articles rated: 2609
23 April 2024 |
|
| | | | |
|
Article overview
| |
|
|
NIR imaging and modeling of the core of M100 | | J.H. Knapen
; R.F. Peletier
; I. Shlosman
; J.E. Beckman
; C.H. Heller
; R.S. de Jong
; | | Date: |
29 Sep 1995 | | Subject: | astro-ph | | Affiliation: | Montreal), R.F. Peletier (Kapteyn), I. Shlosman (Lexington), J.E. Beckman (IAC Tenerife), C.H. Heller (Goettingen), and R.S. de Jong (Durham | | Abstract: | High-resolution NIR and optical images are used to constrain a dynamical model of the circumnuclear star forming (SF) region in the barred galaxy M100 (=NGC 4321). Subarcsecond resolution allowed us to distinguish important morphological details which are easily misinterpreted when using images at lower resolution. Small leading arms observed in our K-band image of the nuclear region are reproduced in the gas flow in our model, and lead us to believe that part of the K light comes from young stars, which trace the gas flow. | | Source: | arXiv, astro-ph/9509153 | | 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:
| |
REGISTER