A Young Planet Search in Visible and IR Light: DN Tau, V836 Tau, and V827 Tau

@article{Prato2008AYP,
  title={A Young Planet Search in Visible and IR Light: DN Tau, V836 Tau, and V827 Tau},
  author={L. Prato and M. Huerta and C. Johns-Krull and N. Mahmud and D. Jaffe and P. Hartigan},
  journal={arXiv: Astrophysics},
  year={2008}
}
  • L. Prato, M. Huerta, +3 authors P. Hartigan
  • Published 2008
  • Physics
  • arXiv: Astrophysics
  • In searches for low-mass companions to late-type stars, correlation between radial velocity variations and line bisector slope changes indicates contamination by large starspots. Two young stars demonstrate that this test is not sufficient to rule out starspots as a cause of radial velocity variations. As part of our survey for substellar companions to T Tauri stars, we identified the ~2 Myr old planet host candidates DN Tau and V836 Tau. In both cases, visible light radial velocity modulation… CONTINUE READING
    9 Citations

    Figures from this paper.

    Evidence against the young hot-Jupiter around BD +20 1790
    • 40
    • PDF
    Rotation periods of exoplanet host stars
    • 26
    • PDF
    Radial velocities with CRIRES - Pushing precision down to 5-10 m/s
    • 44
    • PDF
    Preliminary design of IGRINS (Immersion GRating INfrared Spectrograph)
    • 52
    • PDF

    References

    SHOWING 1-10 OF 29 REFERENCES
    Starspot-Induced Radial Velocity Variability in LkCa 19
    • 28
    • PDF
    The Lick Planet Search: Detectability and Mass Thresholds
    • 260
    • PDF
    Evidence for a Planetary Companion around a Nearby Young Star
    • 37
    • Highly Influential
    • PDF
    No planet for HD 166435
    • 563
    • PDF
    Activity-Related Radial Velocity Variation in Cool Stars
    • 299
    • PDF
    Radial Velocities for 889 Late-Type Stars*
    • 369
    • PDF
    Near-Infrared Photometric Variability of Stars toward the Orion A Molecular Cloud
    • 223
    • PDF
    Magnetospheric accretion-ejection processes in the classical T Tauri star AA Tauri
    • 174
    • PDF