Spectroscopical Masses of Post--AGB Stars

Details Spectroscopical Masses of Post--AGB Stars Spectroscopical Masses of Post--AGB Stars

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001assl..265..271s&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

1

Scientific paper

The literature has been reviewed in search of available spectroscopic parameters for the post-AGB objects. The surface gravity and the effective temperature have been used for determination of spectroscopic masses from comparison with theoretical evolutionary tracks. The derived distribution of masses is relatively narrow and concentrates around 0.55 Msolar in agreement with analogous distributions for central stars of planetary nebulae and white dwarfs.

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