2 research outputs found
Multi-epoch VLBI of a double maser super burst
In a rare and spectacular display, two well-known massive star forming
regions, W49N and G25.65+1.05, recently underwent maser 'super burst' - their
fluxes suddenly increasing above 30,000 and 18,000 Jy, respectively, reaching
several orders of magnitude above their usual values. In quick-response, ToO
observations with the EVN, VLBA and KaVA were obtained constituting a 4 week
campaign - producing a high-cadence multi-epoch VLBI investigation of the maser
emission. The combination of high-resolution, polarisation and flux monitoring
during the burst provides one of the best accounts, to date, of the maser super
burst phenomenon, aiding their use as astrophysical tools. These proceedings
contain the preliminary results of our campaign
Recent updates on the Maser Monitoring Organisation
The Maser Monitoring Organisation (M2O) is a research community of telescope operators, astronomy researchers and maser theoreticians pursuing a joint goal of reaching a deeper understanding of maser emission and exploring its variety of uses as tracers of astrophysical events. These proceedings detail the origin, motivations and current status of the M2O, as was introduced at the 2021 EVN symposium