Other
Scientific paper
Oct 1979
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979pasp...91..659b&link_type=abstract
Astronomical Society of the Pacific, Publications, vol. 91, Oct.-Nov. 1979, p. 659, 660.
Other
17
Carbon Stars, M Stars, Magellanic Clouds, Stellar Spectrophotometry, Star Clusters, Telescopes
Scientific paper
In order to determine which stars near NGC 419 show M-type or carbon-type features, a IV - N plate was taken through a grating-prism combination at the prime-focus of CTIO's 4-m telescope. Seventy eight stars were found in this area, all showing strong CN bands at 7948 A, 8125 A, and 8320 A. From their frequency-per-unit area in the field, three C-type stars appear to be likely members of the cluster. The red stars found near NGC 419 are identified and their properties are presented along with other writers designations.
Blanco Victor M.
Richer Harvey B.
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