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Seismological studies of ZZ Ceti stars - II. Application to the ZZ Ceti class
- Source :
- Repositório Institucional da UFRGS, Universidade Federal do Rio Grande do Sul (UFRGS), instacron:UFRGS
- Publication Year :
- 2009
-
Abstract
- We used the detected pulsation modes and adiabatic pulsation models to do seismology of the class of ZZ Ceti stars and measure the H layer mass for 83 stars. We found the surface hydrogen layer to be within the range 10−9.5 ≥ MH/M* ≥ 10−4, with an average of MH/M* = 10−6.3, which is thinner than the predicted value of MH/M* = 10−4, indicating that the stars lose more mass during their evolution than previously expected. These results are preliminary and do not include the possible effects of realistic C/O profiles on the fits.
Details
- Language :
- English
- Database :
- OpenAIRE
- Journal :
- Repositório Institucional da UFRGS, Universidade Federal do Rio Grande do Sul (UFRGS), instacron:UFRGS
- Accession number :
- edsair.od......3056..c59b716512cf9b4a576b394bba12e27d