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20122025
most citedMagnetic field strengths of hot Jupiters from signals of star-planet interactions

135 citations · 1.7k across the 52 of their papers we have counts for

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Showing 2018Show all

10 papers · 1 filter

astro-ph.SR2018★ 14 cited

Multi-wavelength observations of the EUV variable metal-rich white dwarf GD 394

David J. Wilson, Boris T. Gaensicke, Detlev Koester +13

We present new Hubble Space Telescope (HST) ultraviolet and ground-based optical observations of the hot, metal-rich white dwarf GD 394. Extreme-ultraviolet (EUV) observations in 1…

astro-ph.EP2018★ 39 cited

Evidence of magnetic star-planet interactions in the HD 189733 system from orbitally-phased Ca II K variations

P. Wilson Cauley, Evgenya L. Shkolnik, Joe Llama +2

Magnetic star-planet interactions (SPI) provide a detection method and insight into exoplanet magnetic fields and, in turn, exoplanet interiors and atmospheric environments. These…

astro-ph.EP2018★ 25 cited

K2-140b and K2-180b - Characterization of a hot Jupiter and a mini-Neptune from the K2 mission

J. Korth, Sz. Csizmadia, D. Gandolfi +40

We report the independent discovery and characterization of two K2 planets: K2-180b, a mini-Neptune-size planet in an 8.9-day orbit transiting a V = 12.6 mag, metal-poor ([Fe/H] =$…

astro-ph.EP2018★ 107 cited

Atmospheric dynamics and the variable transit of KELT-9 b

P. Wilson Cauley, Evgenya L. Shkolnik, Ilya Ilyin +3

We present a spectrally and temporally resolved detection of the optical Mg I triplet at 7.8 in the extended atmosphere of the ultra-hot Jupiter KELT-9 b, adding to the list of…

gr-qc2018★ 22 cited

Black hole remnants may exist if Starobinsky inflation occurred

Paul R. Anderson, Mathew J. Binkley, Jillian M. Bjerke +1

Zero temperature black hole solutions to the semiclassical backreaction equations are investigated. Evidence is provided that certain components of the stress-energy tensors for fr…

astro-ph.EP2018★ 48 cited

Dust Production and Depletion in Evolved Planetary Systems

J. Farihi, R. van Lieshout, P. W. Cauley +15

The infrared dust emission from the white dwarf GD 56 is found to rise and fall by 20% peak-to-peak over 11.2 yr, and is consistent with ongoing dust production and depletion. It i…