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IUE ultra-violet spectrophotometry of 15 galactic Wolf-rayet stars.

Schmutz, W.; Nussbaumer, H.; Willis, A. J. +1 more

Low-resolution IUE ultraviolet spectrophotometry is presented of 15 galactic WR stars, covering most subtypes in the WN and WC sequences. The data are presented both as spectral plots and as tabulations of the observed absolute flux distributions covering the wavelength range of 1150-3090 A. The characteristics of these UV WR spectra are discussed…

The ultraviolet spectrum of KQ PUP (Boss 1985).

Altamore, A.; Viotti, R.; Giangrande, A.

The high resolution spectrum of the VV Cep star KQ Pup observed with the IUE satellite during 1979 and 1980 is summarized. More than 600 lines have been identified between 1190 and 3228 A. Two main line systems are present, a broad absorption line system, which includes high ionization lines from N V, C IV, Si IV and Al III, and narrow P Cygni lin…

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

Beckman, J. E.; Selvelli, P. L.; Crivellari, L.

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…

The mid-ultraviolet spectrum of EPS Aur.

Kondo, Y.; Castelli, F.; Hoekstra, R.

An LTE synthetic spectrum with Te = 7800 K and log g = 1 has been computed for the 2455-to-3230 A range of Epsilon Aurigae (F0 1a). This has been compared with the spectra observed with 0.2 A resolution with the IUE experiment and with 0.1 A resolution with the BUSS experiment. As a consequence of this comparison, identifications and abundance val…

UV and visible photometry of the brightest Pleiades stars.

Mauron, N.; Golay, M.

This paper describes 7-color photometric observations of the brightest stars in the Pleiades taken over the last 20 years. These data are analyzed in conjunction with UV photometric and spectroscopic observations made with the OAO-II, IUE satellites and a balloon-borne photometer. Accurate determinations of the interstellar extinction are obtained…