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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4329
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dc.contributor.authorParthasarathy, M-
dc.contributor.authorPottasch, S. R-
dc.date.accessioned2009-02-04T16:23:11Z-
dc.date.available2009-02-04T16:23:11Z-
dc.date.issued1986-01-
dc.identifier.citationAstronomy and Astrophysics, Vol. 154, No. 1 - 2, pp. L16 - L19en
dc.identifier.issn0004-6361-
dc.identifier.urihttp://hdl.handle.net/2248/4329-
dc.description.abstractThe far infrared IRAS measurements of the high galactic latitude F-supergiant HD 161796 and related stars are found to show strong far infrared excesses, due to large amounts of dust around them. For HD 161796 the dust mass is found to be of the order of 10/sup-2M_sun; to 10/sup-3M_sun;, and for HD 101584 it is of the order of 10/sup-3M_sun;. These results suggest that HD 161796 and other similar high galactic latitude F-supergiants have suffered extensive mass loss in the past as a result of superwind phenomenon on their AGB stage of evolution.en
dc.language.isoenen
dc.publisherEuropean Southern Observatoryen
dc.relation.urihttp://adsabs.harvard.edu/abs/1986A%26A...154L..16Pen
dc.subjectFar Infrared Radiationen
dc.subjectSpaceborne Astronomyen
dc.subjectStellar Envelopesen
dc.subjectStellar Mass Ejectionen
dc.subjectSupergiant Starsen
dc.subjectA Starsen
dc.subjectAsymptotic Giant Branch Starsen
dc.subjectB Starsen
dc.subjectF Starsen
dc.subjectInfrared Astronomy Satelliteen
dc.subjectPlanetary Nebulaeen
dc.subjectStellar Evolutionen
dc.subjectStellar Windsen
dc.titleThe far-infrared (IRAS) excess in HD 161796 and related starsen
dc.typeArticleen
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