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.
Bibliographical reference

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

Advertised on:
2
1982
Journal
Astronomy and Astrophysics Supplement Series
Number of authors
3
IAC number of authors
0
Citations
9
Refereed citations
9
Description
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.
Type
Refereed
Main sequence stars
Stellar evolution
Stellar rotation

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