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      EPIC 220501947 b and K2-237 b: two transiting hot Jupiters

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          Abstract

          We report the discovery from K2 of two transiting hot Jupiter systems. EPIC 220501947 (observed in Campaign 8) is a K5 dwarf which hosts a planet slightly smaller than Jupiter, orbiting with a period of 4.0 d. We have made an independent discovery of K2-237 b (Campaign 11), which orbits an F6 dwarf every 2.2 d and has an inflated radius 50 - 60 per cent larger than that of Jupiter. We use high-precision radial velocity measurements, obtained using the HARPS and FIES spectrographs, to measure the planetary masses. We find that EPIC 220501947 b has a similar mass to Saturn, while K2-237 b is a little more massive than Jupiter.

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          IRCS: infrared camera and spectrograph for the Subaru Telescope

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            FastCam: a new lucky imaging instrument for medium-sized telescopes

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              The Structure of Exoplanets

              The hundreds of exoplanets that have been discovered in the past two decades offer a new perspective on planetary structure. Instead of being the archetypal examples of planets, those of our Solar System are merely possible outcomes of planetary system formation and evolution, and conceivably not even terribly common outcomes (although this remains an open question). Here, we review the diverse range of interior structures that are known to, and speculated to, exist in exoplanetary systems -- from mostly degenerate objects that are more than 10 times as massive as Jupiter, to intermediate-mass Neptune-like objects with large cores and moderate hydrogen/helium envelopes, to rocky objects with roughly the mass of the Earth.
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                Author and article information

                Journal
                16 July 2018
                Article
                1807.05865
                41e2e3df-3a4e-42df-9378-c6aae0aeef6b

                http://arxiv.org/licenses/nonexclusive-distrib/1.0/

                History
                Custom metadata
                11 pages, 11 figures, submitted to MNRAS
                astro-ph.EP

                Planetary astrophysics
                Planetary astrophysics

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