Preprint article · Journal article
Characterization of Low-mass K2 Planet Hosts Using Near-infrared Spectroscopy
Ohio State University1
Massachusetts Institute of Technology2
National Space Institute, Technical University of Denmark3
Astrophysics and Atmospheric Physics, National Space Institute, Technical University of Denmark4
University of Texas at Austin5
The University of Chicago6
California Institute of Technology7
We present moderate resolution near-infrared spectra in the H, J, and K band of M-dwarf hosts to candidate transiting exoplanets discovered by NASA’s K2 mission. We employ known empirical relationships between spectral features and physical stellar properties to measure the effective temperature, radius, metallicity, and luminosity of our sample.
Out of an initial sample of 56 late-type stars in K2, we identify 35 objects as M dwarfs. For that subsample, we derive temperatures ranging from 2870 to 4187 K, radii of 0.09–0.83 R⊙, luminosities of -2.67 < log L/L , < -0.67 and [Fe/H] metallicities between −0.49 and 0.51 dex. We then employ the stellar properties derived from spectra, in tandem with the K2 light curves, to characterize their planets.
We report 33 exoplanet candidates with orbital periods ranging from 0.19 to 21.16 days, and median radii and equilibrium temperatures of 2.3 R⊕ and 986 K, respectively. Using planet mass–radius relationships from the literature, we identify seven exoplanets as potentially rocky, although we conclude that probably none reside in the habitable zone of their parent stars.
Language: | English |
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Publisher: | American Astronomical Society |
Year: | 2019 |
Pages: | 15 |
ISSN: | 15383881 , 00046256 , 15384357 and 0004637x |
Types: | Preprint article and Journal article |
DOI: | 10.3847/1538-3881/ab3347 |
ORCIDs: | Mayo, Andrew |
Planetary systems Planets and satellites: fundamental parameters Stars: fundamental parameters Stars: late-type Stars: low-mass Techniques: spectroscopic
astro-ph.EP astro-ph.SR planetary systems planetary systems – planets and satellites: fundamental parameters – stars: fundamental parameters – stars: late-type – stars: low-mass – techniques: spectroscopic planets and satellites: fundamental parameters stars: fundamental parameters stars: late-type stars: low-mass techniques: spectroscopic