M type giants in a Galactic bulge window at L = 0 deg, B = -8 deg

Details M type giants in a Galactic bulge window at L = 0 deg, B = -8 deg M type giants in a Galactic bulge window at L = 0 deg, B = -8 deg

Feb 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987aj.....93..321b&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 93, Feb. 1987, p. 321, 322.

Astronomy and Astrophysics

Astronomy

8

Galactic Bulge, Galactic Structure, Giant Stars, Infrared Windows, M Stars, Milky Way Galaxy, Stellar Spectrophotometry, Absorption Spectra, Galactic Nuclei, Near Infrared Radiation, Stellar Color

Scientific paper

One hundred twenty Galactic bulge giants of type M2 or later are identified in a low-absorption window that includes two areas previously surveyed in B, V colors by van den Bergh and Herbst (1974). The survey reaches past the distance to the galactic center. The observational technique is identical to one already used in Baade's Window and the identifications presented here will allow comparisons of bulge M giants in two different galactocentric distances. Two of the giants found are very likely IRAS point sources.

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