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

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

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997a%26as..123..115n&link_type=abstract

A & A Supplement series, Vol. 123, May II 1997, 115-118.

Other

10

Stars: Carbon, Agb, Post Agb, Variables: Others, Local Group, Galaxies: Sagittarius Dwarf

Scientific paper

A 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 \cite[Azzopardi et al. (1991)]{azz91}. Serendipity provides the suggestion, that their carbon stars might not be located inside, but behind the bulge in the Sagittarius dwarf galaxy. Table 1 and the finding charts of the variable stars are only available in electronic form at the CDS via anonymous {ftp} to cdsarc.u-strasbg.fr (130.79.128.5) or http://cdsweb.u-strabg.fr/Abstract.html.

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