NGC 6826: a unified study of the planetary nebula and its central stars

Details NGC 6826: a unified study of the planetary nebula and its central stars NGC 6826: a unified study of the planetary nebula and its central stars

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011rmxac..40..167f&link_type=abstract

XIII Latin American Regional IAU Meeting (Eds. W. J. Henney & S. Torres-Peimbert) Revista Mexicana de Astronomía y Astrofísica (

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Methodology

Ism: Abundances, Planetary Nebulae: Individual (Ngc 6826), Stars: Abundances, Stars: Atmospheres, Stars: Rotation, Stars: Winds, Outflows

Scientific paper

We present a methodology to obtain a stellar-nebular self-consistent model. Distance is determined using theoretical evolutive tracks of central stars of planetary nebulae. This methodology is applied to study of the galactic planetary nebula NGC 6826. A unified model requieres more work, but its uncertainties are smaller due to their larger number of observational constraints.

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