Physics
Scientific paper
Jan 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003ycat..34001043a&link_type=abstract
VizieR On-line Data Catalog: J/A+A/400/1043. Originally published in: 2003A&A...400.1043A
Physics
Stars: Early-Type, Stars: Supergiant, Spectroscopy
Scientific paper
The table 2 presents the full line identifications of Deneb for the range 3826-5212Å. The far left column contains the letters L and R are a guide to the range of lines whose wings are at least somewhat blended together. The columns are the measured stellar wavelength in Å, the equivalent width (EW) in mÅ, the line depth as a fraction of the continuum height, the line width (FWHM) in Å, the laboratory wavelength in Å, which is the stellar wavelength as corrected for the stellar radial velocity of each spectrum, and the identified atomic lines which cause the observed feature. The stellar and the laboratory wavelengths should be close, but blending and errors can produce discrepancies. Possible identifications are given in parentheses and brackets indicate that an identified line may be contributing to two measured stellar feature.
(3 data files).
Adelman Saul J.
Albayrak Berahitdin
Aydin Cemal
Gulliver Austin F.
Kocer Dursun
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