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Statements

Subject Item
n2:RIV%2F67985815%3A_____%2F11%3A00371959%21RIV12-AV0-67985815
rdf:type
skos:Concept n16:Vysledek
dcterms:description
We use smoothed particle hydrodynamics (SPH) simulations to investigate the gravitational fragmentation of expanding shells through the linear and non-linear regimes. The results are analysed using spherical-harmonic decomposition to capture the initiation of structure during the linear regime, the potential-based method of Smith et al. to follow the development of clumps in the mildly non-linear regime and sink particles to capture the properties of the final bound objects during the highly non-linear regime. In the early, mildly non-linear phase of fragmentation, we find that the clump mass function still agrees quite well with the mass function predicted by the analytic model. We use smoothed particle hydrodynamics (SPH) simulations to investigate the gravitational fragmentation of expanding shells through the linear and non-linear regimes. The results are analysed using spherical-harmonic decomposition to capture the initiation of structure during the linear regime, the potential-based method of Smith et al. to follow the development of clumps in the mildly non-linear regime and sink particles to capture the properties of the final bound objects during the highly non-linear regime. In the early, mildly non-linear phase of fragmentation, we find that the clump mass function still agrees quite well with the mass function predicted by the analytic model.
dcterms:title
The fragmentation of expanding shells - III. Oligarchic accretion and the mass spectrum of fragments The fragmentation of expanding shells - III. Oligarchic accretion and the mass spectrum of fragments
skos:prefLabel
The fragmentation of expanding shells - III. Oligarchic accretion and the mass spectrum of fragments The fragmentation of expanding shells - III. Oligarchic accretion and the mass spectrum of fragments
skos:notation
RIV/67985815:_____/11:00371959!RIV12-AV0-67985815
n16:predkladatel
n17:ico%3A67985815
n3:aktivita
n13:P n13:Z
n3:aktivity
P(LC06014), Z(AV0Z10030501)
n3:cisloPeriodika
4
n3:dodaniDat
n19:2012
n3:domaciTvurceVysledku
n5:4068947 Dale, James E. n5:6877656
n3:druhVysledku
n15:J
n3:duvernostUdaju
n18:S
n3:entitaPredkladatele
n8:predkladatel
n3:idSjednocenehoVysledku
200304
n3:idVysledku
RIV/67985815:_____/11:00371959
n3:jazykVysledku
n7:eng
n3:klicovaSlova
stars formation; ISM bubbles; H II regions
n3:klicoveSlovo
n11:H%20II%20regions n11:ISM%20bubbles n11:stars%20formation
n3:kodStatuVydavatele
GB - Spojené království Velké Británie a Severního Irska
n3:kontrolniKodProRIV
[7F5A0A304C6D]
n3:nazevZdroje
Monthly Notices of the Royal Astronomical Society
n3:obor
n4:BN
n3:pocetDomacichTvurcuVysledku
3
n3:pocetTvurcuVysledku
5
n3:projekt
n10:LC06014
n3:rokUplatneniVysledku
n19:2011
n3:svazekPeriodika
411
n3:tvurceVysledku
Palouš, Jan Smith, R. J. Dale, James E. Wünsch, Richard Whitworth, A.
n3:wos
000287859200010
n3:zamer
n9:AV0Z10030501
s:issn
0035-8711
s:numberOfPages
11
n20:doi
10.1111/j.1365-2966.2010.17844.x