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Misidentified OH/IR Stars

Published online by Cambridge University Press:  25 April 2016

B. M. Lewis  and
P. te Lintel Hekkert
B. M. Lewis
Affiliation:
Arecibo Observatory, PO Box 995 Arecibo, PR 00612, USA
P. te Lintel Hekkert
Affiliation:
Mount Stromlo and Siding Spring Observatories, Private Bag, Weston ACT 2611
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Abstract

Plots of periods against (25μm – 12μm) colour of OH/IR stars suggest that four IRAS sources, that have been associated with known OH/IR stars, either provide anomalous identifications, or are weak rather than regular variables. It is argued here that only one of these cases is an association error. OH15.7+0.8 and OH37.1–0.8 are the new proto–planetary nebula candidates.

Type
Galactic and Stellar
Information
Publications of the Astronomical Society of Australia , Volume 9 , Issue 2 , 1991 , pp. 304 - 305
Copyright
Copyright © Astronomical Society of Australia 1991

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