Are halo carbon stars associated with dwarf spheroidal galaxies?

Details Are halo carbon stars associated with dwarf spheroidal galaxies? Are halo carbon stars associated with dwarf spheroidal galaxies?

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984pasp...96..869v&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 96, Nov. 1984, p. 869, 870.

Astronomy and Astrophysics

Astronomy

3

Carbon Stars, Dwarf Galaxies, Halos, Counting, Galactic Structure

Scientific paper

Star counts have been performed for rings centered on the carbon star at 1 = 69 degrees, b = + 55 degrees at a distance of 60 kpc. The counts were performed in order to determine whether halo carbon stars might be situated in dwarf spheroidal galaxies which are too star-poor to have been recognized as galaxies. The counts were made on a IIIa-J plate baked in forming gas that was exposed for 40 minutes through a 2C filter with the Palomar 1.2-m Schmidt telescope. It is shown that the carbon star is not situated in a dwarf spheroidal galaxy brighter than M(V) = 5.7.

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