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- W96895101 abstract "Through their non-radial, g-mode pulsations, the variable white dwarfs provide us with a means to look beyond their surfaces and peer into their inner compositions and structures. Because of their pulsational complexity, however, we require multi-site campaigns (the Whole Earth Telescope, WET Nather et al. 1990, for example) to gather enough data to isolate and identify their modes of oscillation. The WET has made remarkable progress with the DOVs and DBVs (Winget et al. 1991, Winget et al. 1994), but the DAVs have not readily revealed their interiors, even to long multi-site campaigners." @default.
- W96895101 created "2016-06-24" @default.
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- W96895101 date "1997-01-01" @default.
- W96895101 modified "2023-09-23" @default.
- W96895101 title "Cool DAV Asteroseismology" @default.
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- W96895101 doi "https://doi.org/10.1007/978-94-011-5542-7_66" @default.
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