Abstract
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.
Original language | English |
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Pages (from-to) | 134-138 |
Number of pages | 5 |
Journal | Publications of the Astronomical Society of Australia |
Volume | 16 |
Issue number | 2 |
Publication status | Published - Jul 1999 |
Keywords
- Galaxies: active
- Galaxies: Seyfert
- Planetary nebulae: general