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On the post-common-envelope central star of the planetary nebula NGC 2346

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Academic year: 2019

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Figure

Figure 2. Power spectrum of the radial velocity observations of NGC 2346showing the clear peak at a frequency of 0.0625 d−1 (P = 16 d).
Figure 3. Gaussian fits of the [OIII]5007 Å emission from the PN NGC2346.
Table A1. Radial velocity measurements of the central star of NGC 2346.

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