Can Dust Injected by SNe Explain the NIR-MIR Excess in Young Massive Stellar Clusters?

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F17%3A00484665" target="_blank" >RIV/67985815:_____/17:00484665 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.3847/1538-4357/aa7510" target="_blank" >http://dx.doi.org/10.3847/1538-4357/aa7510</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.3847/1538-4357/aa7510" target="_blank" >10.3847/1538-4357/aa7510</a>

Result language
angličtina
Original language name
Can Dust Injected by SNe Explain the NIR-MIR Excess in Young Massive Stellar Clusters?
Original language description
We present a physically motivated model involving the different processes affecting supernova dust grains as they are incorporated into the thermalized medium within young massive star clusters. The model is used to explain the near- to mid-infrared (NIR-MIR) excess found in such clusters and usually modeled as a blackbody with temperature similar to(400-1000) K. In our approach, dust grains are efficiently produced in the clumpy ejecta of core-collapse supernovae, shattered into small pieces (less than or similar to 0.05 mu m) as they are incorporated into the hot and dense ISM, heated via frequent collisions with electrons and the absorption of energetic photons.
Czech name
—
Czech description
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Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
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OECD FORD branch
10308 - Astronomy (including astrophysics,space science)

Project
<a href="/en/project/GA15-06012S" target="_blank" >GA15-06012S: Multi-Generation Star Clusters</a><br>
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Publication year
2017
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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