EA063
Imaging variable sources from Irbene monitoring program
We propose to observe three methanol maser sources at 6.7 GHz that have been monitored with the Irbene 16m and 32m radio telescopes. Inspection of the single dish spectra and the Torun-Irbene join observations indicates that these sources are significantly variable. Our aims are: i) to derive milliarcsecond morphologies of the emission, ii) to identify cloudlets responsible for the emission changes in the single dish spectra, iii) to put constraints on variability mechanisms going on around these high-mass young stars.
Observation pages at the EVN archive:
Context for this dataThis 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