Possible Post-AGB Stars

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dc.creatorWallerstein, G.
dc.creatorGonzalez, G.
dc.creatorShetrone, M. D.
dc.date2003-05-08
dc.date.accessioned2026-07-07T02:08:26Z
dc.date.available2026-07-07T02:08:26Z
dc.descriptionRadial 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.
dc.identifierhttps://arxiv.org/abs/astro-ph/0305143
dc.identifierhttp://arxiv.org/abs/astro-ph/0305143
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6050
dc.subjectAstrophysics
dc.titlePossible Post-AGB Stars
dc.typetext

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