Diffuse X-rays from PNe with WR-type central stars

Details Diffuse X-rays from PNe with WR-type central stars Diffuse X-rays from PNe with WR-type central stars

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1273..213r&link_type=abstract

17TH EUROPEAN WHITE DWARF WORKSHOP. AIP Conference Proceedings, Volume 1273, pp. 213-218 (2010).

Physics

Hydrodynamics, Nebulae, X-Ray Spectra, Stellar Winds, Hydrodynamics, Physical Properties, X-Ray, Mass Loss And Stellar Winds

Scientific paper

With the help of detailed nebula modeling and X-ray observations, we want to shed light on the enigmatic origin of Wolf-Rayet type central stars of planetary nebulae. This method allows us to assign observed [WC] stars to one of the proposed evolutionary scenarios, attributing the loss of hydrogen to a ``late'', ``very late'', or an ``AGB final'' thermal pulse (LTP, VLTP and AFTP, respectively). We conclude that BD+30° 3639 evolved through an AFTP.

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