Astronomy and Astrophysics – Astrophysics
Scientific paper
May 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26as...88..265a&link_type=abstract
Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 88, no. 2, May 1991, p. 265-275.
Astronomy and Astrophysics
Astrophysics
26
Carbon Stars, Galactic Bulge, Infrared Photometry, Late Stars, Stellar Spectrophotometry, Stellar Color, Stellar Magnitude, Stellar Temperature
Scientific paper
Positions, identification charts, spectra in the wavelength range 4500-7000 A or 4000-7100 A, and equivalent widths of the main lines and bands are presented for the 34 carbon stars that were identified in eight fields of the galactic bulge. Spectrophotometric data in the visible are provided as well as infrared J, H, and K magnitudes for all these objects, and L magnitudes for about half of them. These data are used to derive intrinsic colors, effective temperatures, and bolometric magnitudes.
Azzopardi Marc
Lequeux James
Rebeirot E.
Westerlund Bengt E.
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