dc.citation.endPage |
260 |
- |
dc.citation.number |
1-4 |
- |
dc.citation.startPage |
255 |
- |
dc.citation.title |
ASTROPHYSICS AND SPACE SCIENCE |
- |
dc.citation.volume |
292 |
- |
dc.contributor.author |
Kim, Jongsoo |
- |
dc.contributor.author |
Ryu, Dongsu |
- |
dc.contributor.author |
Hong, Seung Soo |
- |
dc.date.accessioned |
2023-12-22T11:07:30Z |
- |
dc.date.available |
2023-12-22T11:07:30Z |
- |
dc.date.created |
2015-08-26 |
- |
dc.date.issued |
2004 |
- |
dc.description.abstract |
The stratified interstellar medium has been known to be subject to the Parker instability, and the instability has been considered as a plausible mechanism for the formation of giant molecular clouds (GMCs). By presenting our recent efforts to understand the instability through linear analyses and numerical simulations, we raise a negative point of view that the Parker instability alone could not form GMCs |
- |
dc.identifier.bibliographicCitation |
ASTROPHYSICS AND SPACE SCIENCE, v.292, no.1-4, pp.255 - 260 |
- |
dc.identifier.doi |
10.1023/B:ASTR.0000045024.10113.8b |
- |
dc.identifier.issn |
0004-640X |
- |
dc.identifier.scopusid |
2-s2.0-6344282665 |
- |
dc.identifier.uri |
https://scholarworks.unist.ac.kr/handle/201301/18508 |
- |
dc.identifier.url |
http://link.springer.com/article/10.1023%2FB%3AASTR.0000045024.10113.8b |
- |
dc.identifier.wosid |
000224461300030 |
- |
dc.language |
영어 |
- |
dc.publisher |
SPRINGER |
- |
dc.title |
Is the Parker instability a viable mechanism for the formation of giant molecular clouds? |
- |
dc.type |
Article |
- |
dc.description.journalRegisteredClass |
scopus |
- |