Journal
ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES
Volume 145, Issue 2, Pages 269-274Publisher
E D P SCIENCES
DOI: 10.1051/aas:2000242
Keywords
stars : AGB and post-AGB; stars : evolution; stars : early-type; stars : emission-line; stars : atmospheres
Categories
Ask authors/readers for more resources
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.
Authors
I am an author on this paper
Click your name to claim this paper and add it to your profile.
Reviews
Recommended
No Data Available
Share Paper
