UV Spectroscopy of the Central Star of the Planetary Nebula Abell 43

Details UV Spectroscopy of the Central Star of the Planetary Nebula Abell 43 UV Spectroscopy of the Central Star of the Planetary Nebula Abell 43

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1273..231f&link_type=abstract

17TH EUROPEAN WHITE DWARF WORKSHOP. AIP Conference Proceedings, Volume 1273, pp. 231-234 (2010).

Physics

Planetary Nebulae, White Dwarfs, Spectral Analysis, Interstellar Matter, Planetary Nebulae, Faint Blue Stars, White Dwarfs, Degenerate Stars, Nuclei Of Planetary Nebulae, Luminosities, Magnitudes, Effective Temperatures, Colors, And Spectral Classification, Physical Properties

Scientific paper

The central star of the planetary nebula Abell 43 (WD 1751+106) is one
of only four known so-called hybrid PG 1159 stars. These are
hydrogen-deficient due to a late thermal pulse. We present results of a
spectral analysis of FUSE, HST / GHRS, and IUE UV observations by means
of NLTE model-atmosphere techniques.

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