Context. NGC 7538 is a complex massive star-forming region. The region is composed of several radio continuum sources, one of which is IRS 1, a high-mass protostar, from which a 0.3 pc molecular bipolar outflow was detected. Several maser species have been detected around IRS 1. The CH3OH masers have been suggested to trace a Keplerian-disk, while the H2O masers are almost aligned to the outflow. More recent results suggested that the region hosts a torus and potentially a disk, but with a different inclination than the Keplerian-disk that is supposed to be traced by the CH3OH masers. Aims. Tracing the magnetic field close to protostars is fundamental for determining the orientation of the disk/torus. Recent studies showed that duri...
Context. The role of magnetic field in shaping planetary nebulae (PNe), either directly or indirectl...
Context. A low- or intermediate-mass star is believed to maintain a spherical shape throughout the e...
Context. While there is evidence for considerable circular polarization of OH masers in star-forming...
Context. NGC 7538 is a complex massive star-forming region. The region is composed of several radio ...
Context. NGC 7538 is a complex massive star-forming region. The region is composed of several radio ...
Context. IRAS 20126+4104 is a well studied B0.5 protostar that is surrounded by a ~1000 au Keplerian...
International audienceContext: While there is evidence for considerable circular polarization of OH ...
International audienceContext: While there is evidence for considerable circular polarization of OH ...
International audienceContext: While there is evidence for considerable circular polarization of OH ...
International audienceContext: While there is evidence for considerable circular polarization of OH ...
Context: A low-or intermediate-mass star is believed to maintain a spherical shape throughout the ev...
Context. Theoretical simulations and observations at different angular resolutions have shown that m...
Context. A debated topic in star formation theory is the role of magnetic fields during th...
Context. Magnetohydrodynamical simulations show that the magnetic field can drive molecular outflows...
Context. Magnetic fields have only recently been included in theoretical simulations of high-mass st...
Context. The role of magnetic field in shaping planetary nebulae (PNe), either directly or indirectl...
Context. A low- or intermediate-mass star is believed to maintain a spherical shape throughout the e...
Context. While there is evidence for considerable circular polarization of OH masers in star-forming...
Context. NGC 7538 is a complex massive star-forming region. The region is composed of several radio ...
Context. NGC 7538 is a complex massive star-forming region. The region is composed of several radio ...
Context. IRAS 20126+4104 is a well studied B0.5 protostar that is surrounded by a ~1000 au Keplerian...
International audienceContext: While there is evidence for considerable circular polarization of OH ...
International audienceContext: While there is evidence for considerable circular polarization of OH ...
International audienceContext: While there is evidence for considerable circular polarization of OH ...
International audienceContext: While there is evidence for considerable circular polarization of OH ...
Context: A low-or intermediate-mass star is believed to maintain a spherical shape throughout the ev...
Context. Theoretical simulations and observations at different angular resolutions have shown that m...
Context. A debated topic in star formation theory is the role of magnetic fields during th...
Context. Magnetohydrodynamical simulations show that the magnetic field can drive molecular outflows...
Context. Magnetic fields have only recently been included in theoretical simulations of high-mass st...
Context. The role of magnetic field in shaping planetary nebulae (PNe), either directly or indirectl...
Context. A low- or intermediate-mass star is believed to maintain a spherical shape throughout the e...
Context. While there is evidence for considerable circular polarization of OH masers in star-forming...