Search Publications
The winds of O-stars. II. The terminal velocities of stellar winds ofO-type stars.
Pauldrach, A. W. A.; Lamers, H. J. G. L. M.; Groenewegen, M. A. T.
The SEI method (Lamers et al., 1987) is used to obtain P Cygni profiles of the UV resonance lines of C IV, N V, and S IV and of the subordinate UV lines of N IV and C III observed in the spectra of 27 O-type stars. Theoretical profiles which include the turbulence effects agree well with the observations, and they can account for the deep absorpti…
Rotational modulation and flares on RS Canum Venaticorum and BY Draconis stars. XI. Ultraviolet spectral images of AR Lacertae in September 1985.
Linsky, J. L.; Walter, F. M.; Neff, J. E. +1 more
High-resolution IUE SWP and LWP spectra of the bright eclipsing RS CVn system AR Lac, obtained during 40 h of continuous observations on September 18-19, 1985, are compiled and used to derive chromosphere images. The data and results are presented graphically and discussed in detail. The K 0 IV star is found to have a globally brighter trailing he…
The luminous quasar HS 1700+6416 and the shape of the "big bump" below 500 A.
Clavel, J.; Reimers, D.; Wamsteker, W. +5 more
In the course of the Hamburg quasar survey a bright (V = 16.1) high redshift (z = 2.72) quasar has been discovered. Follow-up optical high (0.4 A) and low (6 A) resolution spectrophotometry together with IUE observations are presented. With a luminosity at λ_rest_ = 1450 A, L_1450_ = 6 x 10^32^ erg s^-1^ Hz^-1^, HS1700+6416 is the second most lumi…
Non-LTE analysis of extremly helium-rich stars. I. The hot sdO stars LSE 153, 259 and 263.
Husfeld, D.; Butler, K.; Heber, U. +1 more
Results of a non-LTE fine analysis based mainly on high-resolution CASPEC spectra for three extremely helium-rich sdO stars are discussed in order to explain hydrogen deficiency in single stars. High temperature (Teff = 70,000 to 75,000 K) and a position in the log Teff - log g diagram were found close to the Eddington limit. Various abundance est…
Magnetic structure in cool stars. XVI. Emissions from the outer atmospheres of M-type dwarfs.
Mewe, R.; Rutten, R. G. M.; Schrijver, C. J. +2 more
Consideration is given to emission from the outer atmospheres of M-type dwarfs in several spectral lines originating from the chromosphere, the transition-region, and the soft X-ray emission from the corona. It is shown that M-type dwarfs systematically deviate from relations between flux densities in soft X-rays and chromospheric and transition-r…
The circumstellar gas around beta Pictoris. VIII. Evidence for a clumpy structure of the infalling gas.
Ferlet, R.; Vidal-Madjar, A.; Beust, H. +1 more
In a recent paper, the variable and redshifted circumstellar lines of ionized elements in the UV spectrum of Beta Pictoris were studied. The Al III doublet has been investigated, using both archival and recent IUE spectra of Beta Pic. This larger set of data is used to derive some general characteristics of the variable Al III lines. In particular…
Rotational modulation and flares on RS Canum Venaticorum and BY Draconis.stars. X. The 1981 October 3 flare on V711 Tauri (= HR 1099).
Linsky, J. L.; Simon, T.; Neff, J. E. +5 more
We present a unique set of high resolution spectra of V71 1 Tauri = HR 1099 (G5 V + K1 IV) obtained with both the SWP and LWR cameras of lUE, together with simultaneous 6.4 GHz microwave emission and optical photometry, during a bright flare on 3 October 1981. The electron density of the flaring plasma at 6 104K was about 11011
Ultraviolet flares on II Pegasi.
Doyle, J. G.; Byrne, P. B.; van den Oord, G. H. J.
UV spectroscopic observations of the RS CVn star, II Peg, were obtained in February 1983. The observations show evidence for flare activity in greatly enhanced chromospheric and transition region emission lines. The flare radiation is isolated and the electron pressures of the mean quiescent atmosphere and the two flares are derived from the inter…
The UV silicon spectra of early B stars.
Massa, D.
Equivalent widths of UV silicon lines obtained from high dispersion IUE SWP spectra for a sample of 37 mid- to early B stars are presented. These are compared to other atmospheric diagnostics and to model atmosphere calculations. It is found that some of the UV silicon lines are extremely sensitive to stellar temperature and luminosity over the ra…
Long- and short-term variability of the T Tauri star RY Lupi.
Liseau, R.; Gahm, G. F.; Fischerstrom, C. +1 more
Data are presented on spectroscopic and photometric observations of the T Tauri star RY Lupi carried out since 1981 from the FUV to the IR spectral region. These data show a remarkable kind of variability of the RY Lupi. Namely, the FUV and the IR fluxes, as well as the fluxes in H-alpha and H-beta are relatively constant, while the range in V mag…