When expanding shells fragment?

Number of the records: 1

SYSNO ASEP	0124839
Document Type	C - Proceedings Paper (int. conf.)
R&D Document Type	Conference Paper
Title	When expanding shells fragment?
Author(s)	Ehlerová, Soňa (ASU-R)_{RID, ORCID} Palouš, Jan (ASU-R)_{RID, ORCID}
Source Title	Dynamics of star clusters and the Milky way / Deiters S. ; Fuchs B. ; Just A. ; Spurzem R. ; Wielen R.. - San Francisco : Astronomical Society of the Pacific, 2001
Pages	s. 419-421
Number of pages	2 s.
Action	Dynamics of star clusters and the Milky way
Event date	20.03.2000-24.03.2000
VEvent location	Heidelberg
Country	DE - Germany
Event type	WRD
Language	eng - English
Country	US - United States
Keywords	structure ; ISM bubbles ; ISM supernovae remnants
Subject RIV	BN - Astronomy, Celestial Mechanics, Astrophysics
R&D Projects	KSK1003601 GA AV ČR - Academy of Sciences of the Czech Republic (AV ČR)
CEZ	AV0Z1003909 - ASU-R
Annotation	Using results of the linear perturbation theory we analyse the gravitational stability of expanding shells, both analytically and numerically, and study conditions suitable for the fragmentation of shells.
Workplace	Astronomical Institute
Contact	Anežka Melichárková, bibl@asu.cas.cz, Tel.: 323 620 326
Year of Publishing	2002

Number of the records: 1