We have recently obtained polarimetric data at mm wavelengths with ALMA for the young systems DG Tau and CW Tau, for which the rotation properties of jet and disk have been investigated in previous high angular resolution studies. The motivation was to test the models of magneto-centrifugal launch of jets via the determination of the magnetic configuration at the disk surface. The analysis of these data, however, reveals that self-scattering of dust thermal radiation dominates the polarization pattern. It is shown that even if no information on the magnetic field can be derived in this case, the polarization data are a powerful tool for the diagnostics of the properties and the evolution of dust in protoplanetary disks.European Commission -...
We present 870 mu m ALMA observations of polarized dust emission toward the Class II protoplanetary ...
Context. Polarized continuum emission at millimeter-to-submillimeter wavelengths is usually attribut...
The surfaces of astronomical dust grains are a crucial site for chemical reactions. Observations of ...
We have recently obtained polarimetric data at mm wavelengths with ALMA for the young systems DG Tau...
International audienceWe have recently obtained polarimetric data at mm wavelengths with ALMA for th...
International audienceWe have recently obtained polarimetric data at mm wavelengths with ALMA for th...
International audienceWe have recently obtained polarimetric data at mm wavelengths with ALMA for th...
We have obtained ALMA polarimetric data at 870 microns (Band 7) and 0."2 resolution for the protopla...
We present polarimetric data of CW Tau and DG Tau, two well-known Class II disk/jet systems, obtaine...
We present polarimetric data of CW Tau and DG Tau, two well-known Class II disk/jet systems, obtaine...
International audienceWe present polarimetric data of CW Tau and DG Tau, two well-known Class II dis...
International audienceWe present polarimetric data of CW Tau and DG Tau, two well-known Class II dis...
International audienceWe present polarimetric data of CW Tau and DG Tau, two well-known Class II dis...
We have obtained ALMA polarimetric data at 870 microns (Band 7) and 0."2 resolution for the protopla...
We have obtained ALMA polarimetric data at 870 microns (Band 7) and 0."2 resolution for the protopla...
We present 870 mu m ALMA observations of polarized dust emission toward the Class II protoplanetary ...
Context. Polarized continuum emission at millimeter-to-submillimeter wavelengths is usually attribut...
The surfaces of astronomical dust grains are a crucial site for chemical reactions. Observations of ...
We have recently obtained polarimetric data at mm wavelengths with ALMA for the young systems DG Tau...
International audienceWe have recently obtained polarimetric data at mm wavelengths with ALMA for th...
International audienceWe have recently obtained polarimetric data at mm wavelengths with ALMA for th...
International audienceWe have recently obtained polarimetric data at mm wavelengths with ALMA for th...
We have obtained ALMA polarimetric data at 870 microns (Band 7) and 0."2 resolution for the protopla...
We present polarimetric data of CW Tau and DG Tau, two well-known Class II disk/jet systems, obtaine...
We present polarimetric data of CW Tau and DG Tau, two well-known Class II disk/jet systems, obtaine...
International audienceWe present polarimetric data of CW Tau and DG Tau, two well-known Class II dis...
International audienceWe present polarimetric data of CW Tau and DG Tau, two well-known Class II dis...
International audienceWe present polarimetric data of CW Tau and DG Tau, two well-known Class II dis...
We have obtained ALMA polarimetric data at 870 microns (Band 7) and 0."2 resolution for the protopla...
We have obtained ALMA polarimetric data at 870 microns (Band 7) and 0."2 resolution for the protopla...
We present 870 mu m ALMA observations of polarized dust emission toward the Class II protoplanetary ...
Context. Polarized continuum emission at millimeter-to-submillimeter wavelengths is usually attribut...
The surfaces of astronomical dust grains are a crucial site for chemical reactions. Observations of ...