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Project MK27: Cep-A water maser at 22GHz
See also the methanol line detection at 12GHz of CepA in tab
http://parac.eu/projectmk24.htm
Here we present our results for 22GHz.
Cep-A-25-08-2022-sum1-2
With ever better receiver systems, at present a lot of water masers in CepA are detected on several places. These are all located by Very Long Base Interferometry or VLBI.
It is difficult to cross check the peaks we have on -10.6km/s and -8.7km/s to the tables in literature.
pdf :The magnetic field in the star-forming region Cepheus A.
pdf :EVN observations of the methanol masers in Cep A.
Because of the fact that these radio sources are variable, comparison is difficult when observations are made at different times.
The masers can be associated with rotating rings and outflows.
CepA-ref-Riccardo
Michiel Klaassen Januari 2023