HST Spectroscopy of PG 1159 Stars: the Boundary of the GW VIR Instability Strip

Details HST Spectroscopy of PG 1159 Stars: the Boundary of the GW VIR Instability Strip HST Spectroscopy of PG 1159 Stars: the Boundary of the GW VIR Instability Strip

Mar 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998balta...7...71d&link_type=abstract

Baltic Astronomy, v.7, p.71-82.

Astronomy and Astrophysics

Astronomy

8

Stars: White Dwarfs, Atmospheres, Abundances, Oscillations, Individual: Pg 1159-035, Pg 2131+066, Hs 2324+3944

Scientific paper

Our recent analysis of PG 1159 stars, mainly based on the HST
spectroscopy, is presented. The results allow several conclusions
regarding the boundary of the GW Vir instability strip and the driving
mechanism for these pulsations.

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