Leiden University Scholarly Publications

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An SiO toroid and wide-angle outflow associated with the massive protostar W75N(B)-VLA2
Monitoring of the polarized H2O maser emission around the massive protostars W75N(B)-VLA 1 and W75N(B)-VLA 2
6.7 GHz CH_3OH masers polarization in massive star-forming regions: the flux-limited sample
EVN observations of 6.7 GHz methanol maser polarization in massive star-forming regions. V. Completion of the flux-limited sample
Observational identification of a sample of likely recent common-envelope events
Characterizing the radio continuum nature of sources in the massive star-forming region W75N (B)
ALMA reveals the coherence of the magnetic field geometry in OH 231.8+4.2
Inner dusty envelope of the AGB stars W Hydrae, SW Virginis, and R Crateris using SPHERE/ZIMPOL
ALMA reveals the magnetic field evolution in the high-mass star forming complex G9.62+0.19
Stringent limits on the magnetic field strength in the disc of TW Hya. ALMA observations of CN polarisation
EVN observations of 6.7 GHz methanol maser polarization in massive star-forming regions. IV. Magnetic field strength limits and structure for seven additional sources
Measuring magnetic fields from water masers in the synchrotron protostellar jet in W3(H2O)
The ALMA detection of CO rotational line emission in AGB stars in the Large Magellanic Cloud
EVN observations of 6.7 GHz methanol maser polarization in massive star-forming regions. III. The flux-limited sample
EVN observations of 6.7 GHz methanol maser polarization in massive star-forming regions. II. First statistical results
The magnetic field in the star-forming region Cepheus A. from H_2O maser polarization observations
Further VLBA observations of SiO masers toward Mira variable stars
VLBA observations of SiO masers towards Mira variable stars
VLBI astrometry of circumstellar OH masers: Proper motions and parallaxes of four AGB stars
Circular polarization of water masers in the circumstellar envelopes of late type stars

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