Bibcode
Beckman, J. E.; Crivellari, L.; Selvelli, P. L.
Referencia bibliográfica
Astronomy and Astrophysics Supplement Series, vol. 47, Feb. 1982, p. 295-317.
Fecha de publicación:
2
1982
Número de citas
9
Número de citas referidas
9
Descripción
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.