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Statements

Subject Item
n2:RIV%2F67985815%3A_____%2F01%3A01010092%21RIV%2F2003%2FAV0%2FA01003%2FN
rdf:type
skos:Concept n20:Vysledek
dcterms:description
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. 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.
dcterms:title
When expanding shells fragment? When expanding shells fragment?
skos:prefLabel
When expanding shells fragment? When expanding shells fragment?
skos:notation
RIV/67985815:_____/01:01010092!RIV/2003/AV0/A01003/N
n3:strany
419;421
n3:aktivita
n4:P n4:Z
n3:aktivity
P(KSK1003601), Z(AV0Z1003909)
n3:dodaniDat
n8:2003
n3:domaciTvurceVysledku
n17:8315817 n17:6877656
n3:druhVysledku
n6:D
n3:duvernostUdaju
n19:S
n3:entitaPredkladatele
n7:predkladatel
n3:idSjednocenehoVysledku
702236
n3:idVysledku
RIV/67985815:_____/01:01010092
n3:jazykVysledku
n12:eng
n3:klicovaSlova
structure; - ISM bubbles; - ISM supernovae remnants
n3:klicoveSlovo
n15:-%20ISM%20bubbles n15:-%20ISM%20supernovae%20remnants n15:structure
n3:kontrolniKodProRIV
[B1C241B88662]
n3:mistoKonaniAkce
Heidelberg [DE]
n3:mistoVydani
San Francisco
n3:nazevZdroje
Dynamics of star clusters and the Milky way.
n3:obor
n13:BN
n3:pocetDomacichTvurcuVysledku
2
n3:pocetTvurcuVysledku
2
n3:pocetUcastnikuAkce
0
n3:pocetZahranicnichUcastnikuAkce
0
n3:projekt
n14:KSK1003601
n3:rokUplatneniVysledku
n8:2001
n3:tvurceVysledku
Palouš, Jan Ehlerová, Soňa
n3:typAkce
n10:WRD
n3:zahajeniAkce
2000-03-20+01:00
n3:zamer
n5:AV0Z1003909
s:numberOfPages
2
n18:hasPublisher
Astronomical Society of the Pacific