DOIAbstract
We present 18 years of high resolution and S/N Hα spectroscopy of the Be shell star o An
We present 18 years of high resolution and S/N Hα spectroscopy of the Be shell star o An
Echelle observations are presented and discussed for 23 of the 27 known “normal” shell stars bright...
Context. High-mass X-ray binaries are bright X-ray sources. The high-energy emission is caused by th...
Aims. Spectroscopic, polarimetric, and high spectral resolution interferometric data covering the pe...
We present 18 years of high resolution and S/N H α spectroscopy of the Be shell star o And, obtained...
Context. Emission lines formed in decretion disks of Be stars often undergo long-term cyclic variat...
Context. High-mass X-ray binaries are bright X-ray sources. The high-energy emission is caused by th...
An analysis of numerous homogenized UBV photoelectric observations and red spectra of the Be star f...
We present photometric observations of the field around the optical counterparts of high-mass X-ray ...
International audience66 Oph is a Be star seen under a moderate inclination angle that shows strong ...
66 Oph is a Be star seen under a moderate inclination angle that shows strong variability from UV ...
Context. Emission lines formed in decretion disks of Be stars often undergo long-term cyclic variati...
Aims. We attempt to determine if a dependency on spectral subtype or vsin i exists for stars undergo...
Context. Be/X-ray binaries (BeXRBs) are the most populous class of high-mass X-ray binaries. Their X...
Context. Be/X-ray binaries (BeXRBs) are the most populous class of high-mass X-ray binaries. Their X...
Be stars are B type stars with Balmer emission from a Keplerian decretion disc. It has long been deb...
Echelle observations are presented and discussed for 23 of the 27 known “normal” shell stars bright...
Context. High-mass X-ray binaries are bright X-ray sources. The high-energy emission is caused by th...
Aims. Spectroscopic, polarimetric, and high spectral resolution interferometric data covering the pe...
We present 18 years of high resolution and S/N H α spectroscopy of the Be shell star o And, obtained...
Context. Emission lines formed in decretion disks of Be stars often undergo long-term cyclic variat...
Context. High-mass X-ray binaries are bright X-ray sources. The high-energy emission is caused by th...
An analysis of numerous homogenized UBV photoelectric observations and red spectra of the Be star f...
We present photometric observations of the field around the optical counterparts of high-mass X-ray ...
International audience66 Oph is a Be star seen under a moderate inclination angle that shows strong ...
66 Oph is a Be star seen under a moderate inclination angle that shows strong variability from UV ...
Context. Emission lines formed in decretion disks of Be stars often undergo long-term cyclic variati...
Aims. We attempt to determine if a dependency on spectral subtype or vsin i exists for stars undergo...
Context. Be/X-ray binaries (BeXRBs) are the most populous class of high-mass X-ray binaries. Their X...
Context. Be/X-ray binaries (BeXRBs) are the most populous class of high-mass X-ray binaries. Their X...
Be stars are B type stars with Balmer emission from a Keplerian decretion disc. It has long been deb...
Echelle observations are presented and discussed for 23 of the 27 known “normal” shell stars bright...
Context. High-mass X-ray binaries are bright X-ray sources. The high-energy emission is caused by th...
Aims. Spectroscopic, polarimetric, and high spectral resolution interferometric data covering the pe...
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