The External Heating of Dust in a Homogeneous Spherical Shell

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dc.contributor.authorDwek, Eli
dc.contributor.authorArendt, Richard
dc.date.accessioned2024-10-28T14:30:40Z
dc.date.available2024-10-28T14:30:40Z
dc.date.issued2024-09-10
dc.description.abstractWe present a procedure for calculating the heating of, and the infrared emission from, dust in a homogeneous spherical shell surrounded by a spherically symmetric source of radiation. The results are applicable to newly formed dust either in supernova ejecta or in the circumstellar medium that has been swept up by the expanding shock wave. They can also be applied to the heating and IR emission from dust in clumps or clouds embedded in a homogeneous radiation field.
dc.description.sponsorshipE.D. thanks the Niels Bohr Institute for their hospitality during the completion of the manuscript, which was supported by a VILLUM FONDEN Young Investigator Grant (project number 25501). Work by R.G.A. was supported by NASA under award number 80GSFC21M0002.
dc.description.urihttp://arxiv.org/abs/2409.04391
dc.format.extent5 pages
dc.genrejournal articles
dc.genrepreprints
dc.identifierdoi:10.13016/m2skdj-xzle
dc.identifier.urihttps://doi.org/10.48550/arXiv.2409.04391
dc.identifier.urihttp://hdl.handle.net/11603/36761
dc.language.isoen_US
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Center for Space Sciences and Technology (CSST) / Center for Research and Exploration in Space Sciences & Technology II (CRSST II)
dc.relation.ispartofUMBC Faculty Collection
dc.rightsAttribution-NonCommercial-NoDerivatives 4.0 International CC BY-NC-ND 4.0 Deed
dc.rights.urihttps://creativecommons.org/licenses/by-nc-nd/4.0/
dc.subjectAstrophysics - Astrophysics of Galaxies
dc.titleThe External Heating of Dust in a Homogeneous Spherical Shell
dc.typeText
dcterms.creatorhttps://orcid.org/0000-0001-8403-8548

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