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- W2092142511 abstract "Context. KUV 05134+2605 is one of the 21 pulsating DB white dwarfs (V777 Her or DBV variables) known so far. The detailed investigation of the short-period and low-amplitude pulsations of these relatively faint targets requires considerable observational efforts from the ground, long-term single-site or multi-site observations. The observed amplitudes of excited modes undergo short-term variations in many cases, which makes determining pulsation modes difficult." @default.
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- W2092142511 date "2014-10-01" @default.
- W2092142511 modified "2023-10-15" @default.
- W2092142511 title "Revealing the pulsational properties of the V777 Herculis star KUV 05134+2605 by its long-term monitoring" @default.
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- W2092142511 doi "https://doi.org/10.1051/0004-6361/201423757" @default.
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