Field #3 of the Palomar-Groningen Survey I. Variable stars at the edge of the Sagittarius dwarf galaxy

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dc.creatorNg, Y. K.
dc.creatorSchultheis, M.
dc.date1996-09-19
dc.date.accessioned2026-07-07T02:21:56Z
dc.date.available2026-07-07T02:21:56Z
dc.descriptionA catalogue is presented with variable (RR Lyrae, semiregular and Mira) stars located inside field #3 of the Palomar-Groningen Survey, at the outer edge of the Sagittarius dwarf galaxy. One of the semiregular variables is a carbon star, comparable with those found by Azzopardi et al. (1991). Serendipity provides the suggestion, that their carbon stars might not be located inside, but behind the bulge in the Sagittarius dwarf galaxy.
dc.description3 pages TeX with 3 postscript figures. Table 1 and the finding charts are available on request. Accepted for publication in A&A Supplement Series
dc.identifierhttps://arxiv.org/abs/astro-ph/9609134
dc.identifierhttp://arxiv.org/abs/astro-ph/9609134
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10690
dc.subjectAstrophysics
dc.titleField #3 of the Palomar-Groningen Survey I. Variable stars at the edge of the Sagittarius dwarf galaxy
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