Corpus ID: 16014229

Possible Post-AGB Stars

@article{Wallerstein2003PossiblePS,
  title={Possible Post-AGB Stars},
  author={George Wallerstein and Graciela H. Gonzalez and Matthew D. Shetrone},
  journal={arXiv: Astrophysics},
  year={2003}
}
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. 

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