Asteroseismology of PG 1541 + 651 and BPM 31594 with TESS
Monthly Notices of the Royal Astronomical Society(2022)
摘要
We present the photometric data from TESS for two known ZZ Ceti stars, PG 1541 + 651 and BPM 31594. Before TESS, both objects only had observations from short runs from ground-based facilities, with three and one period detected, respectively. The TESS data allowed the detection of multiple periodicities, 12 for PG 1541 + 651, and six for BPM 31594, which enables us to perform a detailed asteroseismological study. For both objects, we found a representative asteroseismic model with canonical stellar mass ∼0.61M
⊙
and thick hydrogen envelopes, thicker than 10
−5.3
M
*
. The detection of triplets in the Fourier transform also allowed us to estimate mean rotation periods, being ∼22 h for PG 1541 + 651 and 11.6 h for BPM 31594, which is consistent with a range of values reported for other ZZ Ceti stars.
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关键词
surveys,stars: variables: general,white dwarfs
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