Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2805
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dc.contributor.authorReddy, B. E-
dc.contributor.authorParthasarathy, M-
dc.date.accessioned2008-07-22T11:08:24Z-
dc.date.available2008-07-22T11:08:24Z-
dc.date.issued1996-11-
dc.identifier.citationAstronomical Journal Vol. 112, No. 5, pp. 2053 - 2063en
dc.identifier.issn0004-6256-
dc.identifier.urihttp://hdl.handle.net/2248/2805-
dc.description.abstractCCD imaging and BVRI photometry of 14 IRAS sources with far-IR colors similar to planetary nebulae and post-AGB stars are presented. Also results of optical and near -IR spectroscopy of 10 of these candidates are given. From the observed flux distribution from 0.4 μm to 100 μm we find the presence of hot dust component in addition to the cold dust component. The stellar temperatures,luminositics and distances are estimated. We also estimated the parameters of the circumstellar duast envelopes. These results suggest that the 14 IRAS sources considered here are associated wiyh post-AGB supergiants.en
dc.format.extent2136839 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAmerican Astronomical societyen
dc.relation.urihttp://adsabs.harvard.edu/abs/1996AJ....112.2053Ren
dc.subjectplanetary nebulae: generalen
dc.subjectInfrared : starsen
dc.subjectInfrared:interstellar: continuumen
dc.titleCCD Photometry and Spectroscopy of IRAS Sources Having Far-IR Colors Similar to Planetary Nebulaeen
dc.typeArticleen
Appears in Collections:IIAP Publications

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