[[sponsorship]]天文及天文物理研究所[[note]]已出版;[SCI];有審查制度;具代表性[[note]]http://gateway.isiknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=Drexel&SrcApp=hagerty_opac&KeyRecord=0004-637X&DestApp=JCR&RQ=IF_CAT_BOXPLO
Throughout the entire lifetime of a star, it continuously alters the environment. Diverse processes ...
Submillimetre imaging polarimetry is one of the most powerful tools at present for studying magnetic...
Context. Strong, globally-organized magnetic fields are found for a small fraction of O, B, and A st...
International audienceDust polarization observational results are analyzed for the high-mass star fo...
Context. The importance of magnetic fields at the onset of star formation related to the early fragm...
The role of magnetic fields in the high-mass star-forming (HMSF) process has long been debated. In p...
The role played by magnetic field during the formation of high-mass stars is not yet completely und...
Context. The role of magnetic fields in the star formation process is a contentious matter of debate...
Context. The role of magnetic fields during the formation of high-mass stars is not yet fully unders...
To characterize the magnetic field structure of the outflow and core region within a prototypical hi...
Characteristics of the surface magnetic fields of cool stars are usually established with the help o...
Context. A debated topic in star formation theory is the role of magnetic fields during th...
Massive stars (M> 8 M) typically form in parsec-scale molecular clumps that collapse and fragment...
Magnetic fields can be found at the surface of non-degenerate stars all over the HR diagram. Their n...
We highlight distinct and systematic observational features of magnetic field morphologies in polari...
Throughout the entire lifetime of a star, it continuously alters the environment. Diverse processes ...
Submillimetre imaging polarimetry is one of the most powerful tools at present for studying magnetic...
Context. Strong, globally-organized magnetic fields are found for a small fraction of O, B, and A st...
International audienceDust polarization observational results are analyzed for the high-mass star fo...
Context. The importance of magnetic fields at the onset of star formation related to the early fragm...
The role of magnetic fields in the high-mass star-forming (HMSF) process has long been debated. In p...
The role played by magnetic field during the formation of high-mass stars is not yet completely und...
Context. The role of magnetic fields in the star formation process is a contentious matter of debate...
Context. The role of magnetic fields during the formation of high-mass stars is not yet fully unders...
To characterize the magnetic field structure of the outflow and core region within a prototypical hi...
Characteristics of the surface magnetic fields of cool stars are usually established with the help o...
Context. A debated topic in star formation theory is the role of magnetic fields during th...
Massive stars (M> 8 M) typically form in parsec-scale molecular clumps that collapse and fragment...
Magnetic fields can be found at the surface of non-degenerate stars all over the HR diagram. Their n...
We highlight distinct and systematic observational features of magnetic field morphologies in polari...
Throughout the entire lifetime of a star, it continuously alters the environment. Diverse processes ...
Submillimetre imaging polarimetry is one of the most powerful tools at present for studying magnetic...
Context. Strong, globally-organized magnetic fields are found for a small fraction of O, B, and A st...