Planet formation and migration near the silicate sublimation front in protoplanetary disks

@article{Flock2019PlanetFA,
  title={Planet formation and migration near the silicate sublimation front in protoplanetary disks},
  author={Mario Flock and Neal J. Turner and Gijs D. Mulders and Yasuhiro Hasegawa and R. P. Nelson and Bertram Bitsch},
  journal={Astronomy \& Astrophysics},
  year={2019}
}
Context. The increasing number of newly detected exoplanets at short orbital periods raises questions about their formation and migration histories. Planet formation and migration depend heavily on the structure and dynamics of protoplanetary disks. A particular puzzle that requires explanation arises from one of the key results of the Kepler mission, namely the increase in the planetary occurrence rate with orbital period up to 10 days for F, G, K and M stars. Aims. We investigate the… 
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In 2017, the California-Kepler Survey (CKS) published its first data release (DR1) of high-resolution optical spectra of 1305 planet hosts. Refined CKS planet radii revealed that small planets are
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We report the discovery of a Neptune-like planet (LP 714-47 b, P = 4.05204 d, mb = 30.8 ± 1.5M⊕, Rb = 4.7 ± 0.3 R⊕) located in the “hot Neptune desert”. Confirmation of the TESS Object of Interest
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