Context. The low-resolution, Cassegrain mounted, FORS spectropolarimeter of the ESO Very Large Telescope is being extensively used for magnetic field surveys. Some of the new discoveries suggest that relatively strong magnetic fields may play an important role in numerous physical phenomena observed in the atmospheres as well as in the circumstellar environments of certain kinds of stars. Aims. We show in detail how small instabilities or data-reduction inaccuracies represent an alternative explanation for the origin of certain signals of circular polarisation published in recent years. Methods. With the help of analytical calculations we simulate the ob...
Within the context of the collaboration "B fields in OB stars (BOB)", we used the FORS2 low-resoluti...
New determinations of the mean longitudinal magnetic field, of the crossover, and of the mean quadra...
To investigate if magnetic fields are present in Wolf–Rayet stars, we selected a few stars in the Ga...
Context. The low-resolution, Cassegrain mounted, FORS spectropolarimeter of the ESO Very L...
Context. The low-resolution, Cassegrain mounted, FORS spectropolarimeter of the ESO Very Large Teles...
Context. During the last decade, the FORS1 instrument of the ESO Very Large Telescope has been exte...
Context. The ESO archive of FORS1 spectropolarimetric observations may be used to create a homogeneo...
Aims. Recently, several arguments have been presented that favour a scenario in which the ...
Our recent search for the presence of a magnetic field in the bright early A-type supergiant HD 9220...
Context. The FORS1 instrument on the ESO Very Large Telescope was used to obtain low-resolution circ...
International audienceRecent spectropolarimetric studies of seven slowly pulsating B (SPB) and beta ...
International audienceWe have obtained 40 high-resolution circular spectropolarimetric measurements ...
Context. The presence of magnetic fields in O-type stars has been suspected for a long time. The dis...
Within the context of the collaboration “B fields in OB stars” (BOB), we used the FORS2 low-resoluti...
Context. An extremely weak circularly polarized signature was recently discovered in spectral lines ...
Within the context of the collaboration "B fields in OB stars (BOB)", we used the FORS2 low-resoluti...
New determinations of the mean longitudinal magnetic field, of the crossover, and of the mean quadra...
To investigate if magnetic fields are present in Wolf–Rayet stars, we selected a few stars in the Ga...
Context. The low-resolution, Cassegrain mounted, FORS spectropolarimeter of the ESO Very L...
Context. The low-resolution, Cassegrain mounted, FORS spectropolarimeter of the ESO Very Large Teles...
Context. During the last decade, the FORS1 instrument of the ESO Very Large Telescope has been exte...
Context. The ESO archive of FORS1 spectropolarimetric observations may be used to create a homogeneo...
Aims. Recently, several arguments have been presented that favour a scenario in which the ...
Our recent search for the presence of a magnetic field in the bright early A-type supergiant HD 9220...
Context. The FORS1 instrument on the ESO Very Large Telescope was used to obtain low-resolution circ...
International audienceRecent spectropolarimetric studies of seven slowly pulsating B (SPB) and beta ...
International audienceWe have obtained 40 high-resolution circular spectropolarimetric measurements ...
Context. The presence of magnetic fields in O-type stars has been suspected for a long time. The dis...
Within the context of the collaboration “B fields in OB stars” (BOB), we used the FORS2 low-resoluti...
Context. An extremely weak circularly polarized signature was recently discovered in spectral lines ...
Within the context of the collaboration "B fields in OB stars (BOB)", we used the FORS2 low-resoluti...
New determinations of the mean longitudinal magnetic field, of the crossover, and of the mean quadra...
To investigate if magnetic fields are present in Wolf–Rayet stars, we selected a few stars in the Ga...