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Multiwavelength Imaging of Planetary Nebulae: Resolving & Disentangling Structure

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Figure

Fig. 3.1 cont. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .
Figure 1.1: False color images of planetary nebulae. These nebulae represent a medley of mor-phologies from round to highly bipolar
Figure 1.2: Schematic Hertzsprung-Russell (HR) diagram illustrating low mass star evolution fromthe main sequence to becoming a white dwarf, from (Herwig, 2005).
Figure 2.1:Example spectra of BD+30 generated using specextract. Here we have fit the X-ray emission with an optically thin, thermal plasma model, assuming intervening photoelectricabsorption
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