In this thesis I study the magnetic activity of young stars via observations of stellar prominences on single stars and by applying the Zeeman Doppler imaging (ZDI) technique to map the magnetic fields and measure differential rotation of a young binary system. Stellar prominences can be observed as absorption transients in the rotationally broadened chromospheric lines of rapidly rotating stars. Observations of Speedy Mic(K3V) reveal a densely packed prominence system at heights far above the stellar co-rotation radius. Further observations were used to estimate prominence column densities and masses. From very high signal-to-noise observations, loops of emission are found that trace the path of prominences seen transiting the stellar disc...
This thesis presents analyses aimed at understanding the rotational properties of stars at the botto...
This thesis describes an investigation aimed at using spectropolarimetric observations of the magnet...
This thesis presents analyses aimed at understanding the rotational properties of stars at the botto...
In this thesis I study the magnetic activity of young stars via observations of stellar prominences ...
We present the first maps of the surface magnetic fields of a pre-main-sequence binary system. Spect...
International audienceWe present the first maps of the surface magnetic fields of a pre-main-sequenc...
| openaire: EC/H2020/818665/EU//UniSDyn Funding Information: T. W. acknowledges the financial suppor...
We present the first measurements of surface differential rotation on a pre-main-sequence binary sys...
Magnetic fields of cool stars can be directly investigated through the study of the Zeeman effect on...
International audienceContext. Young solar analogs reaching the main sequence experience very strong...
This thesis presents analyses aimed at understanding the rotational properties of stars at the botto...
This thesis describes an investigation aimed at using spectropolarimetric observations of the magnet...
This thesis presents analyses aimed at understanding the rotational properties of stars at the botto...
In this thesis I study the magnetic activity of young stars via observations of stellar prominences ...
We present the first maps of the surface magnetic fields of a pre-main-sequence binary system. Spect...
International audienceWe present the first maps of the surface magnetic fields of a pre-main-sequenc...
| openaire: EC/H2020/818665/EU//UniSDyn Funding Information: T. W. acknowledges the financial suppor...
We present the first measurements of surface differential rotation on a pre-main-sequence binary sys...
Magnetic fields of cool stars can be directly investigated through the study of the Zeeman effect on...
International audienceContext. Young solar analogs reaching the main sequence experience very strong...
This thesis presents analyses aimed at understanding the rotational properties of stars at the botto...
This thesis describes an investigation aimed at using spectropolarimetric observations of the magnet...
This thesis presents analyses aimed at understanding the rotational properties of stars at the botto...