We report the results of Hubble Space Telescope STIS observations of the intriguing luminous blue variable/Wolf-Rayet binary system HD 5980 in the Small Magellanic Cloud. Although its spectral characteristics (WN6) are currently very similar to those observed in 1995 in the FUV, some of the line fluxes continue with the increasing trend observed since the 1980s. The erupting star still dominates the emission-line spectrum, and a radial velocity curve from UV lines is derived, supporting previous estimates of its mass (50 M⊙). A rough estimate of 2 × 10-4 M⊙ yr-1 for the current mass-loss rate of this star is derived. The only spectral lines attributable to the close companion are the very extended P Cygni absorption components of the strong...
We present a study of optical spectra of the Wolf-Rayet star AzV 336a (= SMC WR7) in the Small Magel...
We present observations of the massive transitional star W243 in Westerlund 1 . We find an apparent ...
Observations of W stars in the ultraviolet by OAO 2 and at 750 and 1400 MHz with the Green Bank tele...
The Small Magellanic Cloud multiple system HD 5980 contains a luminous blue variable (LBV) that unde...
Observations of the interstellar and circumstellar absorption components obtained with the Hubble Sp...
Over the past 40 years, the massive luminous blue variable/Wolf-Rayet system HD5980 in the Small Mag...
Observations of the optical spectrum of the Wolf-Rayet eclipsing binary HD 5980 in the Small Magella...
HD 5980 is a unique system containing one massive star (star A) that is apparently entering the lumi...
Observations of the interstellar and circumstellar absorption components obtained with the Hubble Sp...
Over the past 40 years, the massive luminous blue variable/Wolf-Rayet system HD 5980 in the Small Ma...
48 pages, 26 figures, accepted by Revista Mexicana de Astrophysica y AstronomiaInternational audienc...
New spectroscopic observations of the LBV/WR multiple system HD 5980 in the Small Magellanic Cloud a...
We have observed the exceptional SMC star HD 5980 during several runs from 1989 to 1995 at ESO La Si...
The massive Wolf-Rayet stellar system HD 5980 in the Small Magellanic Cloud entered a sudden and bri...
We report a detection of far ultraviolet absorption from the supernova remnant SNR 0057 - 7226 in th...
We present a study of optical spectra of the Wolf-Rayet star AzV 336a (= SMC WR7) in the Small Magel...
We present observations of the massive transitional star W243 in Westerlund 1 . We find an apparent ...
Observations of W stars in the ultraviolet by OAO 2 and at 750 and 1400 MHz with the Green Bank tele...
The Small Magellanic Cloud multiple system HD 5980 contains a luminous blue variable (LBV) that unde...
Observations of the interstellar and circumstellar absorption components obtained with the Hubble Sp...
Over the past 40 years, the massive luminous blue variable/Wolf-Rayet system HD5980 in the Small Mag...
Observations of the optical spectrum of the Wolf-Rayet eclipsing binary HD 5980 in the Small Magella...
HD 5980 is a unique system containing one massive star (star A) that is apparently entering the lumi...
Observations of the interstellar and circumstellar absorption components obtained with the Hubble Sp...
Over the past 40 years, the massive luminous blue variable/Wolf-Rayet system HD 5980 in the Small Ma...
48 pages, 26 figures, accepted by Revista Mexicana de Astrophysica y AstronomiaInternational audienc...
New spectroscopic observations of the LBV/WR multiple system HD 5980 in the Small Magellanic Cloud a...
We have observed the exceptional SMC star HD 5980 during several runs from 1989 to 1995 at ESO La Si...
The massive Wolf-Rayet stellar system HD 5980 in the Small Magellanic Cloud entered a sudden and bri...
We report a detection of far ultraviolet absorption from the supernova remnant SNR 0057 - 7226 in th...
We present a study of optical spectra of the Wolf-Rayet star AzV 336a (= SMC WR7) in the Small Magel...
We present observations of the massive transitional star W243 in Westerlund 1 . We find an apparent ...
Observations of W stars in the ultraviolet by OAO 2 and at 750 and 1400 MHz with the Green Bank tele...