Abstract
Natural OH maser emission originates in the dusty circumstellar envelopes of highly evolved long-period variables and super-giant stars undergoing mass-loss. The OH spectra of such stars, at a microwave frequency of 1,612 MHz, are sharp double-peaked emission line profiles in which the two strongest features have a velocity separation of 5–60 km s−1. Their far infrared colours are typical of sources with colour temperatures below 500 K. Most of the 200 known OH/infrared stars were discovered in systematic OH-line surveys, at 1,612 MHz along the galactic plane1–4, generally using small antennae and having a limiting sensitivity of ∼ 1 Jy. But 40 well-studied sources were readily detected with the IRAS satellite5 at 12, 25 and 60 µm and were characterized by a limited range of infrared colours. A more efficient method for detecting new OH/infrared stars is to begin with IRAS source positions, selected for appropriate infrared colours, and using radio-line observations to confirm the OH properties. We demonstrate the validity of this approach here, using the Arecibo 305 m radio-telescope to confirm the 1,612 MHz line observations of sources in IRAS Circulars 8 and 9 (ref. 6); our present observations identify 21 new OH/infrared stars. The new sources have weaker 1,612 MHz fluxes, bluer (60–25) µm colours and a smaller mean separation between the principal emission peaks than previous samples.
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References
Caswell, J. L. & Haynes, R. F. Mon. Not. R. astr. Soc. 173, 649–669 (1975).
Johansson, L. E. B., Andersson, C., Goss, W. M. & Winnberg, A. Astr. Astrophys. Suppl. 28, 199–210 (1977).
Bowers, P. F. Astr. Astrophys. Suppl. 31, 127–146 (1978).
Baud, B., Habing, H. J., Matthews, H. E. & Winnberg, A. Astr. Astrophys. 95, 156–170 (1981).
Olnon, M. et al. Astrophys. J. 278, L41–44 (1984).
IRAS Circulars 8 & 9 Nature 308, 114 (1984).
Bridle, A. H., Davis, M. M., Fomalont, E. B. & Lequeux, J. Astr. J. 77, 405–443 (1972).
Neugebauer, G. et al. Astrophys. J. 278, L1–L6 (1984).
Elitzur, M., Goldreich, P. & Scoville, N. Astrophys. J. 205, 384–396 (1976).
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Lewis, B., Eder, J. & Terzian, Y. Detection of OH radicals from IRAS sources. Nature 313, 200–202 (1985). https://doi.org/10.1038/313200a0
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DOI: https://doi.org/10.1038/313200a0
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