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The FIR/submillimeter appearance of photoionized disks

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dc.contributor.author Yorke, H. W. en_US
dc.contributor.author Richling, S. en_US
dc.date.accessioned 2004-09-22T22:27:41Z
dc.date.available 2004-09-22T22:27:41Z
dc.date.issued 2001-02-11 en_US
dc.identifier.citation FIRST/Herschel Workshop en_US
dc.identifier.citation San Diego, California, USA en_US
dc.identifier.clearanceno 01-0351 en_US
dc.identifier.uri http://hdl.handle.net/2014/12313
dc.description.abstract The evolution and appearance of circumstellar disks in star forming regions are influenced strongly by the radiation from either the central star itself or close comparison and nearby hot stars. en_US
dc.format.extent 173147 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other star formation circumstellar matter HII regions en_US
dc.title The FIR/submillimeter appearance of photoionized disks en_US


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