Low resolution spectroscopy of hot post-AGB candidates

Citation
M. Parthasarathy et al., Low resolution spectroscopy of hot post-AGB candidates, ASTR AST SS, 145(2), 2000, pp. 269-274
Citations number
46
Categorie Soggetti
Space Sciences
Journal title
ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES
ISSN journal
03650138 → ACNP
Volume
145
Issue
2
Year of publication
2000
Pages
269 - 274
Database
ISI
SICI code
0365-0138(200008)145:2<269:LRSOHP>2.0.ZU;2-O
Abstract
Spectral types are determined from low resolution optical spectra of 40 IRA S sources with far-infrared colours similar to planetary nebulae, The prese nce 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 evolut ion.