The spectra of late-type dwarfs and sub-dwarfs in the near ultraviolet. I - Line identifications

Details The spectra of late-type dwarfs and sub-dwarfs in the near ultraviolet. I - Line identifications The spectra of late-type dwarfs and sub-dwarfs in the near ultraviolet. I - Line identifications

Feb 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26as...47..295b&link_type=abstract

Astronomy and Astrophysics Supplement Series, vol. 47, Feb. 1982, p. 295-317.

Astronomy and Astrophysics

Astrophysics

9

Dwarf Stars, Late Stars, Line Spectra, Near Ultraviolet Radiation, Stellar Spectra, Subdwarf Stars, Absorption Spectra, Atomic Spectra, Iue, Main Sequence Stars, Stellar Evolution, Stellar Rotation, Stellar Spectrophotometry, Ultraviolet Spectra

Scientific paper

Spectra from IUE of 6 main sequence and near main sequence stars from classes A5 to G8, between 2700 A and 2900 A wavelength are described. In toto, some 250 absorption lines are identified. Observed differences in those atomic and ionic multiplets present in each spectrum are shown to be due either to the regular progression in spectral class, or to the smearing effect of stellar rotation.

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