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- W52143240 abstract "Efficient all-sky surveys for OH/IR stars can be completed from 1612 MHz line-searches at the positions of color-selected IRAS sources. This approach can easily detect sources of ~50 mJy, so giving a 20 fold improvement in sensitivity. Results of both a 1612 MHz and a 1665/7 MHz survey from Arecibo are presented. These show that color-selected samples include sources with three distinctly different galactic latitude distributions. Objects with (60–25) µm > -0.9 are rarer than the others, have a narrow distribution about the galactic plane, and so come from short-lived massive progenitors. Far-IR colors of sources in the galactic plane, require adjustment for interstellar extinction." @default.
- W52143240 created "2016-06-24" @default.
- W52143240 creator A5085519001 @default.
- W52143240 date "1987-01-01" @default.
- W52143240 modified "2023-10-03" @default.
- W52143240 title "Identification of OH/IR Stars from Color Selected IRAS Sources" @default.
- W52143240 cites W1992222572 @default.
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- W52143240 doi "https://doi.org/10.1007/978-94-009-3813-7_9" @default.
- W52143240 hasPublicationYear "1987" @default.
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