Possible Post-AGB Stars
classification
🌌 astro-ph
keywords
starspost-agbpotentialradialwereclusterdsphfive
read the original 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.
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