We present the results of optical and near-IR spectroscopic and mid-IR imaging observations of the emission-line star MWC 300. Its properties and evolutionary state are still under debate (a B[e] supergiant or a Herbig Be star). For the first time we detected radial velocity variations of the photospheric lines and found a correlation between them and those of the He
We analyse spectroscopic CCD material obtained at the Haute Provence Observatory. We provide line id...
We present the results of bispectrum speckle interferometry of the B[e] star MWC 349A obtained with ...
Context. Photospheric lines of B-type supergiants show variability in their profile shapes. In addit...
We present the results of optical and near-IR spectroscopic and mid-IR imaging observations of the e...
We present the results of optical and near-IR spectroscopic and near-IR photometric observations of ...
We present both optical high-resolution spectroscopic and photometric observations of the FS CMa typ...
The emission-line object HDE 327083 has long been considered to be one of the most luminous stars in...
We present a study of the high-resolution (R = 60 000) optical spectrum of the B[e] supergiant CI Ca...
Context. We investigated the surroundings of MWC 314 in the framework of the study of hot emission l...
We present a study of the high-resolution ($R=60$ 000) optical spectrum of the B[e] supergiant CI Ca...
We analyse spectroscopic CCD material obtained at the Haute Provence Observatory. We provide identif...
The B[e] phenomenon can be present in stars of different types and at different evolutionary stages....
Context. B[e] supergiants are massive post-main-sequence stars, surrounded by a complex circumstella...
We carried out an analysis of existing multicolor photometry and optical spectroscopy of MWC 342, a ...
Context. MWC 314 is one of the most luminous stars in the Milky Way. Its fundamental parameters are ...
We analyse spectroscopic CCD material obtained at the Haute Provence Observatory. We provide line id...
We present the results of bispectrum speckle interferometry of the B[e] star MWC 349A obtained with ...
Context. Photospheric lines of B-type supergiants show variability in their profile shapes. In addit...
We present the results of optical and near-IR spectroscopic and mid-IR imaging observations of the e...
We present the results of optical and near-IR spectroscopic and near-IR photometric observations of ...
We present both optical high-resolution spectroscopic and photometric observations of the FS CMa typ...
The emission-line object HDE 327083 has long been considered to be one of the most luminous stars in...
We present a study of the high-resolution (R = 60 000) optical spectrum of the B[e] supergiant CI Ca...
Context. We investigated the surroundings of MWC 314 in the framework of the study of hot emission l...
We present a study of the high-resolution ($R=60$ 000) optical spectrum of the B[e] supergiant CI Ca...
We analyse spectroscopic CCD material obtained at the Haute Provence Observatory. We provide identif...
The B[e] phenomenon can be present in stars of different types and at different evolutionary stages....
Context. B[e] supergiants are massive post-main-sequence stars, surrounded by a complex circumstella...
We carried out an analysis of existing multicolor photometry and optical spectroscopy of MWC 342, a ...
Context. MWC 314 is one of the most luminous stars in the Milky Way. Its fundamental parameters are ...
We analyse spectroscopic CCD material obtained at the Haute Provence Observatory. We provide line id...
We present the results of bispectrum speckle interferometry of the B[e] star MWC 349A obtained with ...
Context. Photospheric lines of B-type supergiants show variability in their profile shapes. In addit...