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Statements

Subject Item
n2:RIV%2F67985815%3A_____%2F13%3A00423374%21RIV14-GA0-67985815
rdf:type
skos:Concept n15:Vysledek
dcterms:description
Following the observational and theoretical evidence that points at core-collapse supernovae (SNe) as major producers of dust, here we calculate the hydrodynamics of the matter reinserted within young and massive super stellar clusters under the assumption of gas and dust radiative cooling. The large SN rate expected in massive clusters allows for a continuous replenishment of dust immersed in the high temperature thermalized reinserted matter and warrants a stationary presence of dust within the cluster volume during the type II SN era. We first show that such a balance determines the range of the dust-to-gas-mass ratio, and thus the dust cooling law. Following the observational and theoretical evidence that points at core-collapse supernovae (SNe) as major producers of dust, here we calculate the hydrodynamics of the matter reinserted within young and massive super stellar clusters under the assumption of gas and dust radiative cooling. The large SN rate expected in massive clusters allows for a continuous replenishment of dust immersed in the high temperature thermalized reinserted matter and warrants a stationary presence of dust within the cluster volume during the type II SN era. We first show that such a balance determines the range of the dust-to-gas-mass ratio, and thus the dust cooling law.
dcterms:title
Dusty Supernovae Running the Thermodynamics of the Matter Reinserted within Young and Massive Super Stellar Clusters Dusty Supernovae Running the Thermodynamics of the Matter Reinserted within Young and Massive Super Stellar Clusters
skos:prefLabel
Dusty Supernovae Running the Thermodynamics of the Matter Reinserted within Young and Massive Super Stellar Clusters Dusty Supernovae Running the Thermodynamics of the Matter Reinserted within Young and Massive Super Stellar Clusters
skos:notation
RIV/67985815:_____/13:00423374!RIV14-GA0-67985815
n15:predkladatel
n16:ico%3A67985815
n6:aktivita
n9:I n9:P
n6:aktivity
I, P(GAP209/12/1795)
n6:cisloPeriodika
2
n6:dodaniDat
n8:2014
n6:domaciTvurceVysledku
n13:6877656 n13:4068947
n6:druhVysledku
n7:J
n6:duvernostUdaju
n19:S
n6:entitaPredkladatele
n10:predkladatel
n6:idSjednocenehoVysledku
70745
n6:idVysledku
RIV/67985815:_____/13:00423374
n6:jazykVysledku
n14:eng
n6:klicovaSlova
dust; extinction; galaxie
n6:klicoveSlovo
n12:dust n12:extinction n12:galaxie
n6:kodStatuVydavatele
US - Spojené státy americké
n6:kontrolniKodProRIV
[49F5A4B3CB1B]
n6:nazevZdroje
Astrophysical Journal
n6:obor
n17:BN
n6:pocetDomacichTvurcuVysledku
2
n6:pocetTvurcuVysledku
6
n6:projekt
n18:GAP209%2F12%2F1795
n6:rokUplatneniVysledku
n8:2013
n6:svazekPeriodika
778
n6:tvurceVysledku
Martinez-Gonzalez, S. Munoz-Tunon, C. Wünsch, Richard Silich, S. Palouš, Jan Tenorio-Tagle, G.
n6:wos
000327762800074
s:issn
0004-637X
s:numberOfPages
6
n4:doi
10.1088/0004-637X/778/2/159