The Physical Characteristics of Close Binary Central Stars of Planetary Nebulae

Details The Physical Characteristics of Close Binary Central Stars of Planetary Nebulae The Physical Characteristics of Close Binary Central Stars of Planetary Nebulae

Jan 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aas...21725610h&link_type=abstract

American Astronomical Society, AAS Meeting #217, #256.10; Bulletin of the American Astronomical Society, Vol. 43, 2011

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Scientific paper

The number of detected close binary stars in planetary nebulae has increased dramatically in the past several years and is now reaching the level at which statistically significant trends may be made discussed. Several of the important parameters we would like to know are binary fraction of central stars, system classifications, binary parameters (such as inclination), and correlations between the binary and its surrounding planetary nebula. I
will describe the sample of known close binary central stars
in relation to other close binaries with a white dwarf, including cataclysmic variables, supernova Ia progenitors, and double degenerate systems. I will also review the system parameters for well studied systems and relate these, where possible, to their associated nebulae.

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