THE IMPACT OF STELLAR ROTATION ON THE DETECTABILITY OF HABITABLE PLANETS AROUND M DWARFS

Stellar activity and rotation frustrate the detection of exoplanets through the radial velocity technique. This effect is particularly of concern for M dwarfs, which can remain magnetically active for billions of years. We compile rotation periods for late-type stars and for the M dwarf planet-host...

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Bibliographic Details
Main Authors: Newton, Elisabeth R. (Author), Irwin, Jonathan (Author), Charbonneau, David (Author), Dittmann, Jason A. (Author), Berta-Thompson, Zach (Author)
Other Authors: MIT Kavli Institute for Astrophysics and Space Research (Contributor), Berta-Thompson, Zachory K (Contributor)
Format: Article
Language:English
Published: IOP Publishing, 2017-04-21T21:00:15Z.
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