DUSTY SUPERNOVAE RUNNING THE THERMODYNAMICS OF THE MATTER REINSERTED WITHIN YOUNG AND MASSIVE SUPER STELLAR CLUSTERS

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 larg...

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Veröffentlicht in:The Astrophysical journal 2013-12, Vol.778 (2), p.1-6, Article 159
Hauptverfasser: Tenorio-Tagle, Guillermo, Silich, Sergiy, Martinez-Gonzalez, Sergio, MUNOZ-TUNON, CASIANA, PALOUS, JAN, Wunsch, Richard
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Sprache:eng
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