We present time-resolved spectroscopy of the Be star HD 76534, which was observed to have an Ha outburst in 1995, when the line went from photospheric absorption to emission at a level of more than two times the continuum within 2.5 hours. To investigate the short-term behaviour of the spectrum of HD 76534 we have obtained 30 spectra within two hours real-time and searched for variations in the spectrum.Within the levels of statistical significance, no variabilitywas found. Rather than periodic on short time scales, the H behaviour seems to be commonly episodic on longer (> 1 year) time scales, as an assessment of the existing data on theH line and the Hipparcos photometry suggests. HD 76534 underwent only 1 photometric outburst in the 3 ye...
We have investigated the report of Tamura and Takeuti that the H alpha line of the F-type post-AGB s...
We present H band (1.53 μm-1.69 μm) spectra of 57 isolated Be stars of spectral types O9-B9 and lumi...
Aims.We obtained the first long, homogenous time-series of V2104 Cyg, consisting of 679 datapoints,...
We present time-resolved spectroscopy of the Be star HD 76534, which was observed to have an Ha outb...
We present three seasons of photometric observations and one season of intensive high-dispersion spe...
Some results of long time spectral monitoring of the Herbig Ae/Be star MWC 614 (HD 179218) are prese...
The B[e] phenomenon can be present in stars of different types and at different evolutionary stages....
Aims. We attempt to determine if a dependency on spectral subtype or vsin i exists for stars undergo...
Variability is a commonly observed property of classical Be stars (CBe) stars. In extreme cases, com...
We present the results of high-resolution spectroscopic observations of the pre–main-sequence Herbig...
International audienceWe present the first Far Ultraviolet Spectroscopic Explorer (FUSE) spectrum of...
A reliable determination of the basic physical properties and variability patterns of hot emission-l...
Astronomy and Astrophysics 529 (2011): A34 reproduced with permission from Astronomy & AstrophysicsA...
We report the results of high-resolution spectroscopic observations obtained in 2000–2014. The goals...
With the aim of contributing to the understanding of the disk formation process in Be stars, we purs...
We have investigated the report of Tamura and Takeuti that the H alpha line of the F-type post-AGB s...
We present H band (1.53 μm-1.69 μm) spectra of 57 isolated Be stars of spectral types O9-B9 and lumi...
Aims.We obtained the first long, homogenous time-series of V2104 Cyg, consisting of 679 datapoints,...
We present time-resolved spectroscopy of the Be star HD 76534, which was observed to have an Ha outb...
We present three seasons of photometric observations and one season of intensive high-dispersion spe...
Some results of long time spectral monitoring of the Herbig Ae/Be star MWC 614 (HD 179218) are prese...
The B[e] phenomenon can be present in stars of different types and at different evolutionary stages....
Aims. We attempt to determine if a dependency on spectral subtype or vsin i exists for stars undergo...
Variability is a commonly observed property of classical Be stars (CBe) stars. In extreme cases, com...
We present the results of high-resolution spectroscopic observations of the pre–main-sequence Herbig...
International audienceWe present the first Far Ultraviolet Spectroscopic Explorer (FUSE) spectrum of...
A reliable determination of the basic physical properties and variability patterns of hot emission-l...
Astronomy and Astrophysics 529 (2011): A34 reproduced with permission from Astronomy & AstrophysicsA...
We report the results of high-resolution spectroscopic observations obtained in 2000–2014. The goals...
With the aim of contributing to the understanding of the disk formation process in Be stars, we purs...
We have investigated the report of Tamura and Takeuti that the H alpha line of the F-type post-AGB s...
We present H band (1.53 μm-1.69 μm) spectra of 57 isolated Be stars of spectral types O9-B9 and lumi...
Aims.We obtained the first long, homogenous time-series of V2104 Cyg, consisting of 679 datapoints,...