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Orientation Effects in Bipolar Planetary Nebulae
Published online by Cambridge University Press: 26 May 2016
Abstract
Using a sample of 29 bipolar Planetary Nebulae (BPNe) we show correlations between the luminosity and SED shape with the inclination to the line of sight of the objects polar axes. The presence of an equatorial “doughnut” of material around the central object can explain both these correlations and also and the bipolar shape.
- Type
- Part VII: Nebular Morphology and Dynamics
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- Copyright © Astronomical Society of the Pacific 2003