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Detection of rotationally excited OH emission toward the probable young planetary nebular Vy 2-2

Journal Article · · Astrophys. J.; (United States)
DOI:https://doi.org/10.1086/163364· OSTI ID:5307735
A search for 4.7 and 6.0 GHz rotationally excited OH emission in OH/Miras, OH/IR stars, Herbig-Haro objects, Herbig Ae and Be stars, and compact planetary nebulae has been performed. Many of the objects were surveyed in all seven of the lambda doublet hyperfine transitions in the /sup 2/product/sub 3/2/, J = 5/2 and /sup 2/product/sub 1//sub ///sub 2/, J = 1/2 rotational states. In general, this is the most comprehensive and sensitive search for circumstellar rotationally excited OH yet performed. Only one new detection was made, but that was of 6035 MHz emission from the interesting object Vy 2-2. This object is a probable compact planetary nebula surrounded by a fossil molecular envelope from the progenitor red giant. The object was previously known to have a 1612 MHz ground-state OH maser. A complete summary of all observations is given. We discuss the excitation conditions and a number of pumping schemes that could explain the Vy 2-2 masers and the negative results for excited-state OH masers in the other sources. The morphology of the Vy 2-2 envelope as indicated by the velocity structure of the 6035 MHz emissions is also discussed.
Research Organization:
Department of Astronomy, University of Illinois, Urbana
OSTI ID:
5307735
Journal Information:
Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 295:1; ISSN ASJOA
Country of Publication:
United States
Language:
English