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- W2950875376 abstract "Maser emission from water, methanol, silicon monoxide and other molecules can reach brightness temperatures ≫1010 K. Such observations can achieve sub-pc precision for discs around black holes or sub-au scale interactions in protostellar discs and the regions where evolved star winds reach escape velocity. Ultra-high resolution maser observations also provide photon statistics, for fundamental physics experiments. RadioAstron has shown the success – and limitations – of cm-wave maser observations on scales ≪1 mas with sparse baseline coverage. ALMA, APEX and earlier single dish searches have found a wealth of mm and sub-mm masers, some of which probably also attain high brightness temperatures. Masers are ideal for high-resolution observations throughout the radio regime and we need to consider the current lessons for the best observational strategies to meet specific science cases." @default.
- W2950875376 created "2019-06-27" @default.
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- W2950875376 date "2020-01-01" @default.
- W2950875376 modified "2023-10-18" @default.
- W2950875376 title "Masers: Precision probes of molecular gas" @default.
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- W2950875376 doi "https://doi.org/10.1016/j.asr.2019.05.052" @default.
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