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- W30404791 abstract "O-rich circumstellar dust shells that do not exhibit 1612 MHz masers (Lewis 1992), despite appropriate IR colors and 1612 MHz sensitivity, are known as OH/IR star color mimics. Since previous studies of mimics depend on samples with a limited IR spectral type and color range, we use the data collected for poster III-8 to identify the mimics in an all-sky sample of bright IRAS sources with S(25) > 100 Jy and (60-25)μm < 0.0: this expands on Gaylard et al. (1989), and benefits from the greater quantity of maser data now and a wider IR color range." @default.
- W30404791 created "2016-06-24" @default.
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- W30404791 date "1997-01-01" @default.
- W30404791 modified "2023-10-16" @default.
- W30404791 title "OH/IR star color mimics with S(25) > 100 Jy" @default.
- W30404791 cites W1966687406 @default.
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- W30404791 doi "https://doi.org/10.1017/s0074180900131304" @default.
- W30404791 hasPublicationYear "1997" @default.
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