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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4637
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dc.contributor.authorFujii, T-
dc.contributor.authorNakad, Y-
dc.contributor.authorParthasarathy, M-
dc.date.accessioned2009-07-14T11:56:45Z-
dc.date.available2009-07-14T11:56:45Z-
dc.date.issued2001-08-
dc.identifier.citationSzczerba, R. and Garny, S. K., eds., Post-AGB objects as a phase of stellar evolution, Astrophysics and Space Science Library, Vol. 265, Proceedings of the Torun Workshop held July 5 - 7, 2000, pp. 111 – 114en
dc.identifier.isbn0-7923-7145-3-
dc.identifier.urihttp://hdl.handle.net/2248/4637-
dc.descriptionRestricted Access-
dc.description.abstractThe transition from AGB to post-AGB stars was investigated using the H-band monitoring of these objects for four years. The Mira-type pulsations were found only in the restricted area in the IRAS two color diagram. The non-variable sources occupy the region close to the AGB variables. A new class of post-AGB variables was discovered beyond the non-variables. They are probably crossing the instability strip on their rapid evolution to the planetary nebula stage.en
dc.language.isoenen
dc.publisherKluwer Academic Publishersen
dc.relation.ispartofseriesAstrophysics and Space Science Library; Vol. 265-
dc.relation.urihttp://adsabs.harvard.edu/abs/2001ASSL..265..111Fen
dc.subjectLight Variabilityen
dc.subjectIRAS Sourcesen
dc.subjectVariables in Late AGBen
dc.subjectEarly Post-AGB Phaseen
dc.titleLight variability of color selected IRAS sources: variables in late AGB and early post-AGB phaseen
dc.typeArticleen
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