Publication:
Dust in External Galaxies

dc.contributor.authorCalzetti, D
dc.contributor.departmentUniversity of Massachusetts - Amherst
dc.date2023-09-23T03:11:47.000
dc.date.accessioned2024-04-26T08:30:48Z
dc.date.available2024-04-26T08:30:48Z
dc.date.issued2009-01-01
dc.descriptionThis is the pre-published version harvested from ArXiv. The published version is located at http://www.aspbooks.org/a/volumes/article_details/?paper_id=30949
dc.description.abstractExisting (Spitzer Space Telescope) and upcoming (Herschel Space Telescope) facilities are deepening our understanding of the role of dust in tracing the energy budget and chemical evolution of galaxies. The tools we are developing while exploring the local Universe will in turn become pivotal in the interpretation of the high redshift Universe when near--future facilities (the Atacama Large Millimeter Array [ALMA], the Sub--Millimeter Array [SMA], the Large Millimeter Telescope [LMT], the James Webb Space Telescope [JWST]), and, possibly, farther--future ones, will begin operations.
dc.description.pages214
dc.identifier.urihttps://hdl.handle.net/20.500.14394/3543
dc.relation.ispartofAstronomical Society of the Pacific Conference Series
dc.relation.urlhttps://scholarworks.umass.edu/cgi/viewcontent.cgi?article=1954&context=astro_faculty_pubs&unstamped=1
dc.source.issue414
dc.source.statuspublished
dc.subjectAstrophysics and Astronomy
dc.titleDust in External Galaxies
dc.typearticle
dc.typearticle
digcom.contributor.authorisAuthorOfPublication|email:calzetti@astro.umass.edu|institution:University of Massachusetts - Amherst|Calzetti, D
digcom.identifierastro_faculty_pubs/971
digcom.identifier.contextkey1773703
digcom.identifier.submissionpathastro_faculty_pubs/971
dspace.entity.typePublication
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