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- W1525489969 abstract "A four-year search for 86-GHz SiO and H2O maser emission towards about 20 unidentified OH/IR objects and about 35 optically identified variable stars has yielded information on the temporal variations of many of these sources. The SiO maser emission is noted to behave differently in OH/IR objects as compared with Mira variables. An attempt is made to explain the appearance of strong masers in both vibrational states solely at the 43 GHz transition, under the assumption that an intrinsically weak pump mechanism generates weak (v=1, J=2-1) emission." @default.
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- W1525489969 date "1986-05-01" @default.
- W1525489969 modified "2023-09-23" @default.
- W1525489969 title "SiO and H2O maser emission in OH/IR objects and late-type variable stars" @default.
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