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- W2964184485 abstract "The intense line emission of OH masers is a perfect tracer of regions where new stars are born aswell as of evolved stars, shedding large amounts of processed matter into the interstellar medium.From SKA deep surveys at 18 cm, where the maser lines from the ground-state of the OHmolecule arise, we predict the discovery of more than 20000 sources of stellar and interstellarorigin throughout the Galaxy. The study of this maser emission has many applications, includingthe determination of magnetic field strengths from polarisation measurements, studies of stellarkinematics using the precisely determined radial velocities, and distance determinations fromVLBI astrometry. A new opportunity to study shocked gas in different galactic environments isexpected to arise with the detection of lower luminosity masers. For the first time, larger numbersof OH masers will be detected in Local Group galaxies. New insights are expected in structureformation in galaxies by comparing maser populations in galaxies of different metallicity, as boththeir properties as well as their numbers depend on it. With the full capabilities of SKA, furthermaser transitions such as from excited OH and from methanol will be accessible, providing newtools to study the evolution of star-forming regions in particular." @default.
- W2964184485 created "2019-07-30" @default.
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- W2964184485 date "2015-05-29" @default.
- W2964184485 modified "2023-09-26" @default.
- W2964184485 title "OH masers in the Milky Way and Local Group galaxies in the SKA era" @default.
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- W2964184485 doi "https://doi.org/10.22323/1.215.0125" @default.
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