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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3743
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dc.contributor.authorPottasch, S. R-
dc.contributor.authorParthasarathy, M-
dc.date.accessioned2008-09-20T11:38:17Z-
dc.date.available2008-09-20T11:38:17Z-
dc.date.issued1988-03-
dc.identifier.citationAstronomy and Astrophysics , Vol. 192, No. 1 - 2, pp. 182 - 186en
dc.identifier.issn0004-6361-
dc.identifier.urihttp://hdl.handle.net/2248/3743-
dc.description.abstractThe far-infrared IRAS excesses are found in ten luminous F-G stars. The far-IR fluxes from these stars are due to large amounts of dust around them. The far-IR flux distribution, far-IR luminosities and dust masses are similar to those in observed planetary nebulae. The mass of the dust around HD 187885 and HD 179821 is of the order of 10-2M_sun;. These ten stars may be in the AGB - post-AGB stage of evolution.en
dc.language.isoenen
dc.publisherEuropean Southern Observatoryen
dc.relation.urihttp://adsabs.harvard.edu/abs/1988A%26A...192..182Pen
dc.subjectF starsen
dc.subjectFar infrared radiationen
dc.subjectG starsen
dc.subjectInfrared sources (astronomy)en
dc.subjectStellar luminosityen
dc.subjectAsymptotic giant branch starsen
dc.subjectGiant starsen
dc.subjectInfrared astronomy satelliteen
dc.subjectPlanetary nebulaeen
dc.subjectStellar envelopesen
dc.titleThe far-infrared (IRAS) excess in luminous F-G starsen
dc.typeArticleen
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