Astronomy and Astrophysics – Astrophysics
Scientific paper
2004-05-14
Publ.Astron.Soc.Austral.21:334-343,2004
Astronomy and Astrophysics
Astrophysics
17 pages, 5 figures. Submitted to PASA
Scientific paper
10.1071/AS04039
This paper presents (H-alpha + [NII]) imaging and spectroscopy of a previously unknown, highly evolved planetary nebula of low excitation. It was discovered serendipitously from AAO/UKST H-alpha Survey images as part of a project to exploit the survey data and has evaded detection by previous surveys due to very low surface brightness. It is a remarkably annular planetary nebula, some 19' across, making it one of the largest examples of its type. We estimate a radius of 1.5 pc and a distance of 550pc as derived from a new H-alpha surface brightness - radius relation. PFP 1 has near perfect circular symmetry, broken only at the NW edge which is coupled with significantly increased (H-alpha + [NII]) intensity. This indicates an early stage of an interaction with the interstellar medium. A blue central star candidate has been identified from the SuperCOSMOS Sky Survey data.
Frew David J.
Parker Quentin A.
Pierce Michael J.
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