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OH emission from early-type emission-line stars with large infrared excesses

Journal Article · · Astrophys. J.; (United States)
DOI:https://doi.org/10.1086/157099· OSTI ID:6094351
We present the results of a search for ground-state OH emission from 23 early-type emission-line stars with large infrared excesses. The objects were searched at 1612, 1665, and 1667 MHz with the 300 m Arecibo telescope. We detected one new object, Vy 2--2, and confirmed the results of Fix and Mutel for the peculiar OH source M 1--92. The 1612 MHz profile for Vy 2--2 displays a single, strong, asymmetric feature about 10 km s/sup -1/ wide. Vy 2--2 is also an infrared source and a thermal radio continuum source, and has been classified as a planetary nebula of stellar appearance . If the latter classification is correct, it is the first planetary nebula detected in OH. The association of 1612 MHz OH emission and the infrared spectrum suggest that the pump mechanism for Vy 2--2 is far-infrared radiation. Vy 2--2 may represent a planetary nebula in the process of formation. The bipolar nebula M 1--92 has remained unchanged in intensity since 1973. Its evolutionary state is not known. The stars HK Ori and LkH..cap alpha.. 208, suggested as possible weak OH emitters by Lepine and Nguyen-Quang-Rieu, were not detected.
Research Organization:
David Dunlap Observatory, University of Toronto
OSTI ID:
6094351
Journal Information:
Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 230:2; ISSN ASJOA
Country of Publication:
United States
Language:
English