Low resolution spectroscopy of hot post-AGB candidates

dc.contributor.author	Parthasarathy, M
dc.contributor.author	Vijapurkar, J
dc.contributor.author	Drilling, J. S
dc.date.accessioned	2008-09-02T10:48:09Z
dc.date.available	2008-09-02T10:48:09Z
dc.date.issued	2000-08
dc.identifier.citation	Astronomy and Astrophysics Supplement Series, Vol. 145, No. 2, pp. 269 - 274	en
dc.identifier.issn	0365-0138
dc.identifier.uri	http://hdl.handle.net/2248/3323
dc.description.abstract	Spectral types are determined from low resolution optical spectra of 40 IRAS sources with far-infrared colours similar to planetary nebulae. The presence of circumstellar dust, high galactic latitude, and early supergiant or giant spectral type, sometimes with emission in the Balmer lines, indicate that some of these stars are low mass stars in the post-AGB stage of evolution. Based on observations obtained at the Cerro Tololo Inter-American Observatory (CTIO), Chile.	en
dc.language.iso	en	en
dc.publisher	EDP Sciences	en
dc.relation.uri	http://dx.doi.org/10.1051/aas:2000242	en
dc.subject	Stars: AGB and Post-AGB	en
dc.subject	Stars: Evolution	en
dc.subject	Stars: Early-Type	en
dc.subject	Stars: Emission-Line	en
dc.subject	Stars: Atmospheres	en
dc.title	Low resolution spectroscopy of hot post-AGB candidates	en
dc.type	Article	en