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The Optically Resolved Planetary Nebula/OH Maser Vy 2-2*

Published online by Cambridge University Press:  19 July 2016

R. Falomo  and
F. Sabbadin
R. Falomo
Affiliation:
Asiago Astrophysical Observatory, 36012 Asiago (VI), Italy
F. Sabbadin
Affiliation:
Asiago Astrophysical Observatory, 36012 Asiago (VI), Italy

Abstract

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Vy 2-2 is, to our knowledge, the only planetary nebula exhibiting OH emission, indicating that it is a very young PN still enveloped by the neutral shell of the progenitor AGB star.

Type
V. Origin of Planetaries
Information
Symposium - International Astronomical Union , Volume 131: Planetary Nebulae , 1989 , pp. 444
Copyright
Copyright © Kluwer 1989