Spitzer and Herschel studies of dust in supernova remnants in the Small Magellanic Cloud

Spitzer and Herschel studies of dust in supernova remnants in the Small Magellanic Cloud

With the entire Small Magellanic Cloud (SMC) mapped by the Spitzer Space Telescope and Herschel Space Observatory, we were able to search 8-250 μm images in order to identify infrared (IR) emission associated with SMC supernova remnants (SNRs). A valid detection had to correspond with known X-ray, H...

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Bibliographic Details
Main Authors: Ayley, V. (Author), Barlow, M.J (Author), Chawner, H. (Author), Filipović, M.D (Author), Gomez, H.E (Author), Matsuura, M. (Author), Priestley, F.D (Author), Reid, W. (Author), Rigby, A. (Author)
Format: Article
Language:English
Published: Oxford University Press 2022
Subjects:
Carrier concentration
Dust
Dust emission
Dust extinctions
dust, extinction
Electron density measurement
Electrons
Galaxies
galaxies: individual: Small Magellanic Cloud
Galaxies: individual: small Magellanic cloud
Hydrogen
ISM: individual object: DEM s103, NGC 346, ITK 25
ISM: individual objects
ISM: individual objects: DEM S103, NGC 346, ITK 25
ISM: supernova remnants
Pulsars
shock waves
Shock waves
Shock-waves
Spitzer
Supernova remnants
Supernovae
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