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

Bibcode
1982A&AS...47..295B
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
Revista
Astronomy and Astrophysics Supplement Series
Número de autores
3
Número de autores del IAC
0
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.
Tipo
Con árbitro
Estrellas de la secuencia principal
Evolución estelar
Rotación estelar

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