Masses of Central Stars of Planetary Nebulae

Details Masses of Central Stars of Planetary Nebulae Masses of Central Stars of Planetary Nebulae

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001assl..265..167g&link_type=abstract

Post-AGB Objects as a Phase of Stellar Evolution, Proceedings of the Toruń Workshop held July 5-7, 2000. Edited by R. Szczerba a

Astronomy and Astrophysics

Astrophysics

Scientific paper

We present the masses of central stars of 44 planetary nebulae (PN),
obtained from measured [OIII] expansion velocities and derived from the
dynamical ages. The stellar core mass distribution is narrow, peaking at
0.61 Msolar. We discuss the correlations between central
stars of PN (CSPN) masses and other stellar and nebular parameters.

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