The fragmentation of expanding shells: cloud formation rates and masses.
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F02%3A01030140" target="_blank" >RIV/67985815:_____/02:01030140 - isvavai.cz</a>
Result on the web
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DOI - Digital Object Identifier
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Alternative languages
Result language
angličtina
Original language name
The fragmentation of expanding shells: cloud formation rates and masses.
Original language description
The gravitational instability of expanding shells is discussed. Linear and nonlinear terms are included in an analytical solution in the static and homogeneous medium. The authors discuss the interaction of modes and give the time needed for fragmentation. Results of simulations are compared to observation.
Czech name
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Czech description
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Classification
Type
D - Article in proceedings
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
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Result continuities
Project
Result was created during the realization of more than one project. More information in the Projects tab.
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>Z - Vyzkumny zamer (s odkazem do CEZ)
Others
Publication year
2002
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Article name in the collection
Extragalactic star clusters.
ISBN
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ISSN
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e-ISSN
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Number of pages
3
Pages from-to
675-677
Publisher name
Astronomical Society of the Pacific
Place of publication
San Francisco
Event location
Pucon [CL]
Event date
Mar 12, 2001
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
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