ED046
EVN mapping of 6.7 GHz maser in accretion burst candidate.
We propose to map the structure of the OH, CH3OH and H2O maser lines towards a high-mass protostar at the early stage of the burst seen in the 6.7GHz methanol maser. The goals of the project are (i) to measure the position of the masers, (ii) to examine the maser structure at mas scale and location of the flaring emission in order to constrain the physical properties of maser regions, (iii) to provide a case study for the causes of the maser variability.
Observation pages at the EVN archive:
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