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ISOPHOT Observations of Dust Disks Around Main Sequence (Vega-Like) Stars

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dc.contributor.author Walker, H. J. en_US
dc.contributor.author Heinrichsen, I. en_US
dc.date.accessioned 2004-09-25
dc.date.available 2004-09-25
dc.date.issued 1998-09 en_US
dc.identifier.citation ICARUS en_US
dc.identifier.citation USA en_US
dc.identifier.clearanceno 98-1597 en_US
dc.identifier.uri http://hdl.handle.net/2014/20585
dc.description.abstract The photometer (ISOPHOT) on the Infrared Space Observatory (ISO) has proved to be invaluable for investigating the dust around main sequence stars (both prototypes and candidate Vega-like Stars). en_US
dc.format.extent 652585 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other photometer ISOPHOT infrared observations infrared space observatory ISO vega-like stars dust disk planet formation extrasolar planets en_US
dc.title ISOPHOT Observations of Dust Disks Around Main Sequence (Vega-Like) Stars en_US


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