ED048
EVN mapping of 6.7 GHz maser in G85.41
We propose to map the structure of 6.7 GHz methanol maser emission towards high-mass protostars G85.41 and Cep A during the bursts. The goals of the project are (i) to uncover the structure of emission in the possible early stages of burst, (ii) to examine the hypotheses on the origin of variability and (iii) to study the origin of the quasi-periodic behaviour of the low-luminosity features in Cep A.
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