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  2. PRODOTTI RICERCA INAF
  3. 3 CONTRIBUTI IN ATTI DI CONVEGNO (Proceedings)
  4. 3.01 Contributi in Atti di convegno
Please use this identifier to cite or link to this item: http://hdl.handle.net/20.500.12386/24433
Title: Dust grains from the heart of supernovae
Authors: Bocchio, Marco
MARASSI, Stefania
SCHNEIDER, RAFFAELLA 
BIANCHI, SIMONE 
LIMONGI, Marco 
CHIEFFI, ALESSANDRO 
Issue Date: 2016
Volume: Supernova Remnants: An Odyssey in Space after Stellar Death
First Page: 134
Abstract: Dust grains are classically thought to form in the winds of asymptotic giant branch (AGB) stars. However, there is increasing evidence today for dust formation in supernovae (SNe). To establish the relative importance of these two classes of stellar sources of dust, it is important to know the fraction of freshly formed dust in SN ejecta that is able to survive the passage of the reverse shock and be injected in the interstellar medium. We have developed a new code (GRASH_Rev) which follows the newly-formed dust evolution throughout the supernova explosion until the merging of the forward shock with the circumstellar ISM. We have considered four well studied SNe in the Milky Way and Large Magellanic Cloud: SN1987A, CasA, the Crab Nebula, and N49. For all the simulated models, we find good agreement with observations and estimate that between 1 and 8% of the observed mass will survive, leading to a SN dust production rate of (3.9± 3.7)×10^(-4) MM_{☉})/yr in the Milky Way. This value is one order of magnitude larger than the dust production rate by AGB stars but insufficient to counterbalance the dust destruction by SNe, therefore requiring dust accretion in the gas phase.
Conference Name: Supernova Remnants: An Odyssey in Space after Stellar death
Conference Place: Chania, Crete, Greece
Conference Date: June 6-11, 2016
URI: http://hdl.handle.net/20.500.12386/24433
URL: http://snr2016.astro.noa.gr/homepage.php/
Bibcode ADS: 2016sros.confE.134B
Fulltext: open
Appears in Collections:3.01 Contributi in Atti di convegno

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