Light variability of color selected IRAS sources: variables in late AGB and early post-AGB phase

dc.contributor.author	Fujii, T
dc.contributor.author	Nakad, Y
dc.contributor.author	Parthasarathy, M
dc.date.accessioned	2009-07-14T11:56:45Z
dc.date.available	2009-07-14T11:56:45Z
dc.date.issued	2001-08
dc.identifier.citation	Szczerba, 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 – 114	en
dc.identifier.isbn	0-7923-7145-3
dc.identifier.uri	http://hdl.handle.net/2248/4637
dc.description	Restricted Access
dc.description.abstract	The 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.iso	en	en
dc.publisher	Kluwer Academic Publishers	en
dc.relation.ispartofseries	Astrophysics and Space Science Library; Vol. 265
dc.relation.uri	http://adsabs.harvard.edu/abs/2001ASSL..265..111F	en
dc.subject	Light Variability	en
dc.subject	IRAS Sources	en
dc.subject	Variables in Late AGB	en
dc.subject	Early Post-AGB Phase	en
dc.title	Light variability of color selected IRAS sources: variables in late AGB and early post-AGB phase	en
dc.type	Article	en