A New Timescale for Period Change in the Pulsating DA White Dwarf WD 0111+0018
arXiv:1302.1875 · doi:10.1088/0004-637X/766/1/42
Abstract
We report the most rapid rate of period change measured to date for a pulsating DA (hydrogen atmosphere) white dwarf (WD), observed in the 292.9 s mode of WD 0111+0018. The observed period change, faster than 10^{-12} s/s, exceeds by more than two orders of magnitude the expected rate from cooling alone for this class of slow and simply evolving pulsating WDs. This result indicates the presence of an additional timescale for period evolution in these pulsating objects. We also measure the rates of period change of nonlinear combination frequencies and show that they share the evolutionary characteristics of their parent modes, confirming that these combination frequencies are not independent modes but rather artifacts of some nonlinear distortion in the outer layers of the star.
10 pages, 6 figures, accepted for publication in The Astrophysical Journal
References in corpus (6)
- Pulsating White Dwarf Stars and Precision Asteroseismology
- Toward ensemble asteroseismology of ZZ Ceti stars with fully evolutionary models
- The rate of cooling of the pulsating white dwarf star G117B15A: a new asteroseismological inference of the axion mass
- Mapping the ZZ Ceti Instability Strip: Discovery of 6 New Pulsators
- Fine Grid Asteroseismology of R548 and G117-B15A
- Empirical Determination of Convection Parameters in White Dwarfs I : Whole Earth Telescope Observations of EC14012-1446
Cited by in corpus (12)
- Pulsating white dwarfs: new insights
- White Dwarf Rotation as a Function of Mass and a Dichotomy of Mode Linewidths: Kepler Observations of 27 Pulsating DA White Dwarfs Through K2 Campaign 8
- Amplitude and frequency variations of oscillation modes in the pulsating DB white dwarf star KIC~08626021: The likely signature of nonlinear resonant mode coupling
- Long-term eclipse timing of white dwarf binaries: an observational hint of a magnetic mechanism at work
- Precision asteroseismology of the pulsating white dwarf GD 1212 using a two-wheel-controlled Kepler spacecraft
- Detections and Constraints on White Dwarf Variability from Time-Series GALEX Observations
- Limits on Mode Coherence in Pulsating DA White Dwarfs Due to a Non-static Convection Zone
- Pulsating low-mass white dwarfs in the frame of new evolutionary sequences: IV. The secular rate of period change
- Timing by Stellar Pulsations as an Exoplanet Discovery Method
- Seismic test of the mass-radius relationship of hydrogen-atmospheric white dwarf stars
- Relativistic Corrections in White Dwarf Asteroseismology
- A triplet of the only pulsation mode detected in the DAV star G132-12