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Two New Planetary Nebulae and an AGN in the Galactic Plane

Published online by Cambridge University Press:  05 March 2013

S. H. Beer  and
A. E. Vaughan
S. H. Beer
Affiliation:
School of Mathematics, Physics, Computing and Electronics, Macquarie University, North Ryde, NSW 2109, Australia
A. E. Vaughan
Affiliation:
School of Mathematics, Physics, Computing and Electronics, Macquarie University, North Ryde, NSW 2109, Australia
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Abstract

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A search for planetary nebulae was carried out using candidates selected by their infrared colours and 5 GHz radio emission. One new planetary nebula was identified on the basis of its small angular size, strong [O iii] emission and infrared colours. Another object, known as the possible planetary nebula Wray 16–28, is similarly identified as a planetary nebula. An undiscovered AGN was also found, and is classed as a Seyfert 2 galaxy on the basis of its strong O iii emission, linewidths of ∼500 km s−1, and 5 GHz radio flux. Low-resolution optical spectra are presented and distance estimates discussed.

Keywords

planetary nebulae: generalgalaxies: activegalaxies: Seyfert
Type
Research Article
Information
Publications of the Astronomical Society of Australia , Volume 16 , Issue 2 , 1999 , pp. 134 - 138
Copyright
Copyright © Astronomical Society of Australia 1999

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