SIMBAD references

2014ApJ...792..112A - Astrophys. J., 792, 112 (2014/September-2)

A spin-orbit alignment for the hot Jupiter HATS-3b.


Abstract (from CDS):

We have measured the alignment between the orbit of HATS-3b (a recently discovered, slightly inflated Hot Jupiter) and the spin axis of its host star. Data were obtained using the CYCLOPS2 optical-fiber bundle and its simultaneous calibration system feeding the UCLES spectrograph on the Anglo-Australian Telescope. The sky-projected spin-orbit angle of λ = 3°±25° was determined from spectroscopic measurements of the Rossiter-McLaughlin effect. This is the first exoplanet discovered through the HATSouth transit survey to have its spin-orbit angle measured. Our results indicate that the orbital plane of HATS-3b is consistent with being aligned to the spin axis of its host star. The low obliquity of the HATS-3 system, which has a relatively hot mid F-type host star, agrees with the general trend observed for Hot Jupiter host stars with effective temperatures >6250 K to have randomly distributed spin-orbit angles.

Abstract Copyright:

Journal keyword(s): planets and satellites: dynamical evolution and stability - stars: individual: HATS-3 - techniques: radial velocities

Simbad objects: 20

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