Context. Once ALMA full polarization capabilities are offered, it will become possible to perform detailed studies of polarized maser emission towards star-forming regions and late-type stars, such as ( post-) asymptotic giant branch stars and young planetary nebulae. To derive the magnetic field orientation from maser linear polarization, a number of conditions involving the rate of stimulated emission R, the decay rate of the molecular state Gamma, and the Zeeman frequency g Omega need to be satisfied. Aims. The goal of this work is to investigate if SiO, H2O and HCN maser emission within the ALMA frequency range can be detected with observable levels of fractional linear polarization in the regime where the Zeeman frequency is greater th...
Context: A low-or intermediate-mass star is believed to maintain a spherical shape throughout the ev...
Through the observations and the analysis of maser polarization it is possible to measure the magnet...
We study the polarization of the SiO maser emission in a representative sample of evolved stars in o...
Context. Once ALMA full polarization capabilities are offered, it will become possible to perform de...
Context. Once ALMA full polarization capabilities are offered, it will become possible to perform de...
Context. Once ALMA full polarization capabilities are offered, it will become possible to perform de...
Once ALMA full polarization capabilities are offered, (sub-)mm polarization studies will enter a new...
Polarized emission from astrophysical masers can provide important information about physical condit...
Polarized emission from astrophysical masers can provide important information about physical condit...
Polarized emission from astrophysical masers can provide important information about physical condi...
Context. A low- or intermediate-mass star is believed to maintain a spherical shape throughout the e...
Context. Ground-state OH maser emission from late-type stars is usually polarized and rema...
Context. Ground-state OH maser emission from late-type stars is usually polarized and rema...
Aims.We study the polarization of the SiO maser emission in a representative sample of evolved stars...
Aims.We study the polarization of the SiO maser emission in a representative sample of evolved stars...
Context: A low-or intermediate-mass star is believed to maintain a spherical shape throughout the ev...
Through the observations and the analysis of maser polarization it is possible to measure the magnet...
We study the polarization of the SiO maser emission in a representative sample of evolved stars in o...
Context. Once ALMA full polarization capabilities are offered, it will become possible to perform de...
Context. Once ALMA full polarization capabilities are offered, it will become possible to perform de...
Context. Once ALMA full polarization capabilities are offered, it will become possible to perform de...
Once ALMA full polarization capabilities are offered, (sub-)mm polarization studies will enter a new...
Polarized emission from astrophysical masers can provide important information about physical condit...
Polarized emission from astrophysical masers can provide important information about physical condit...
Polarized emission from astrophysical masers can provide important information about physical condi...
Context. A low- or intermediate-mass star is believed to maintain a spherical shape throughout the e...
Context. Ground-state OH maser emission from late-type stars is usually polarized and rema...
Context. Ground-state OH maser emission from late-type stars is usually polarized and rema...
Aims.We study the polarization of the SiO maser emission in a representative sample of evolved stars...
Aims.We study the polarization of the SiO maser emission in a representative sample of evolved stars...
Context: A low-or intermediate-mass star is believed to maintain a spherical shape throughout the ev...
Through the observations and the analysis of maser polarization it is possible to measure the magnet...
We study the polarization of the SiO maser emission in a representative sample of evolved stars in o...