Landing page for project EK061

We propose high-resolution observations of 2 methanol maser sources G32.03+0.06, G35.20-1.74 (W48) at 6.7 GHz using the European VLBI Network (EVN). These masers have been systematically monitored over the past five years with the Irbene 16 m and 32 m radio telescopes [1]. Selected sources have different variability types periodic, quasi-periodic, long-term dimming. Our primary objectives are to investigate the proper motions, variability mechanisms, source morphology, and cloudlet structure evolution of these masers. We aim to identify the physical processes driving maser variability and improve our understanding of the underlying astrophysical conditions.

This data is part of the archive of VLBI data maintained by JIVE on behalf of the EVN, a network of radio telescopes located primarily in Europe and Asia, with additional antennas in South Africa. The EVN archive itself has the DOI https://doi.org/10.17616/R3Z197