Timescale for the variation of the 539 s pulsation mode of PG 1159-035
Costa J. E. S., Kepler S. O., Winget D. E.
Open Astronomy · 1995
doi:10.1515/astro-1995-0308 (opens in a new tab)
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Abstract
We have analyzed all time-series photometry obtained for the pre-white dwarf PG 1159-035 since 1979 in order to measure the timescale of period variation for its second largest pulsation mode.The solution is not unique, but the best value is P = (-0.82±0.04)x 10 -11 ss _1 .
Abstract licence: CC BY-NC-ND
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