Radio-flaring Ultracool Dwarf Population Synthesis

@article{Route2017RadioflaringUD,
  title={Radio-flaring Ultracool Dwarf Population Synthesis},
  author={M. Route},
  journal={arXiv: Solar and Stellar Astrophysics},
  year={2017}
}
  • M. Route
  • Published 2017
  • Physics
  • arXiv: Solar and Stellar Astrophysics
Over a dozen ultracool dwarfs (UCDs), low-mass objects of spectral types $\geq$M7, are known to be sources of radio flares. These typically several-minutes-long radio bursts can be up to 100\% circularly polarized and have high brightness temperatures, consistent with coherent emission via the electron cyclotron maser operating in $\sim$kG magnetic fields. Recently, the statistical properties of the bulk physical parameters that describe these UCDs have become adequately described to permit… Expand

Figures from this paper

Exoplanet transits with next-generation radio telescopes
Radio Stars: from kHz to THz

References

SHOWING 1-10 OF 77 REFERENCES
THE 5 GHz ARECIBO SEARCH FOR RADIO FLARES FROM ULTRACOOL DWARFS
Discovery of Radio Emission from the Tight M8 Binary LP 349–25
THE ARECIBO DETECTION OF THE COOLEST RADIO-FLARING BROWN DWARF
Volume-limited radio survey of ultracool dwarfs
A Survey for Hα Emission from Late L Dwarfs and T Dwarfs
Flaring up All Over—Radio Activity in Rapidly Rotating Late M and L Dwarfs
A mini-survey of ultracool dwarfs at 4.9 GHz
The Radio Activity-Rotation Relation of Ultracool Dwarfs
...
1
2
3
4
5
...