High-gravity central stars
classification
🌌 astro-ph
keywords
starscentralhigh-gravityallowanalysesapparentlyatmosphereexhibited
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NLTE spectral analyses of high-gravity central stars by means of state-of-the-art model atmosphere techniques provide information about the precursor AGB stars. The hydrogen-deficient post-AGB stars allow investigations on the intershell matter which is apparently exhibited at the stellar surface. We summarize recent results from imaging, spectroscopy, and spectropolarimetry.
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