The state and future of WET as an instrument

Articles in the same Issue

1. Contents
2. Contents
3. List of Participants
4. Proceedings of the Fifth Wet Workshop, August 15–20, 1999
5. Introduction
6. Preface
7. The state and future of WET as an instrument
8. Asteroseismological constraints on the extent and cause of the pre-white dwarf instability strip
9. The effect of ³He diffusion on the pulsational spectra of DBV models
10. Nonlinear behavior of the pulsating white dwarf GD 358
11. The temperature of the hot DB GD 190
12. The location of the driving region in white dwarf pulsators
13. identification in pulsating white dwarfs using the HST
14. Light curves and time-resolved spectroscopy of ZZ Ceti stars
15. Frequency stabilities of two pulsating white dwarfs
16. BPM 37093: preliminary results from XCOV 16 and XCOV 17
17. Mode identification of BPM 37093 with the HST
18. Time-resolved spectroscopy of BPM 37093 and PG 1336-018
19. The ZZ Ceti instability strip revisited
20. The ML1/α = 2 instability strip of ZZ Ceti stars
21. PG 1541+650: A new ZZ Ceti white dwarf
22. Origin of the combination frequences in the pulsation spectra of white dwarfs
23. Asteroseismology of Delta Scuti stars
24. Preliminary δ Scuti star catalog
25. Spectral analysis of four multi-mode pulsating sdB stars