The Case low-dispersion northern sky survey. VII - Late-type stars

Details The Case low-dispersion northern sky survey. VII - Late-type stars The Case low-dispersion northern sky survey. VII - Late-type stars

Apr 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apjs...66..387s&link_type=abstract

Astrophysical Journal Supplement Series (ISSN 0067-0049), vol. 66, April 1988, p. 387-390. NSF-supported research.

Astronomy and Astrophysics

Astronomy

40

Carbon Stars, Late Stars, Northern Sky, Sky Surveys (Astronomy), Stellar Magnitude, Stellar Spectra, Faint Objects, Halos, M Stars

Scientific paper

Positions, approximate red magnitudes, and finding charts are provided for 132 faint red stars that show definite or strongly suspected carbon or late M-type spectra. These stars, with apparent red magnitudes ranging from 9 to 17, lie in a roughly 1000 square degree area of sky at high northern Galactic latitudes defined by the approximate boundaries 8h15m < R.A. <17h30m and +29° < decl. < +38°. They were identified on low-dispersion objective-prism plates taken with the Burrell Schmidt telescope at Kitt Peak.

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