Possible Post-AGB Stars
Astrophysics
2007-05-23 v1
Abstract
Radial velocities were measured for 5 potential post-AGB stars, two in the globular cluster NGC 1851 and three in the dSph galaxy Ursa Minor. All five potential PAGB stars were found to be radial velocity non-members.
Cite
@article{arxiv.astro-ph/0305143,
title = {Possible Post-AGB Stars},
author = {G. Wallerstein and G. Gonzalez and M. D. Shetrone},
journal= {arXiv preprint arXiv:astro-ph/0305143},
year = {2007}
}
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