Timing Analysis of the Periodic Radio and Optical Brightness Variations of the Ultracool Dwarf, TVLM 513-46546

@article{Wolszczan2014TimingAO,
  title={Timing Analysis of the Periodic Radio and Optical Brightness Variations of the Ultracool Dwarf, TVLM 513-46546},
  author={A. Wolszczan and M. Astronomy and Astrophysics and T. O. S. University and Center for Exoplanets and Habitable Worlds and Northrop Grumman Mission Systems},
  journal={The Astrophysical Journal},
  year={2014},
  volume={788},
  pages={23}
}
We describe the arrival time measurements and timing modeling of the periodic radio flares and optical brightness variations of the M9 ultracool dwarf, TVLM 513-46546. We confirm the stability of the observed period and determine its best-fit value to be 7054.468±0.007 s over the last 7 years, based on both the new and archival radio observations and the archival optical data. The period, when measured separately for the radio flare and the optical periodicities, is the same to within ±0.02 s… Expand

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