Extreme Solar Systems

By Debra A. Fischer, F. Rasio, F. A. Thorsett, A. Wolszczan. 2008

155 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/b2a6170e06ed186540f10b409286bd2c6dff01c4

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Citations in the corpus

ON THE FORMATION OF HOT JUPITERS IN STELLAR BINARIES (2012, background): “…hand recent studies suggest that the frequency of giant planets in close binaries (< 100AU) is significantly lower then in the overall population (Eggenberger et al. 2008, 2011), indicating that distant stellar perturbers may be important in the production of HJs. Recent measurements of the…”
The HARPS search for southern extra-solar planets - XVII. Super-Earth and Neptune-mass planets in multiple planet systems HD 47 186 and HD 181 433 (2008, background): “In the planet population synthesis calculations of Mordasini et al. (2008a) based on the core accretion scenario, a large number of hot-Neptunian and Super-Earth planets as the ones presented here are predicted to exist at small distances from the host star.”
ATMOSPHERIC CIRCULATION OF HOT JUPITERS: COUPLED RADIATIVE-DYNAMICAL GENERAL CIRCULATION MODEL SIMULATIONS OF HD 189733b and HD 209458b (2008, unknown): “…seen in published 3D simulations that force the ﬂow with a simpliﬁed Newtonian heating/cooling scheme, which relaxes the temperature toward the radiative-equilibrium temperature proﬁle over the expected radiative timescale (Showman et al. 2008a; Fortney et al. 2006a; Cooper & Showman 2005, 2006).”
The Eighteenth Data Release of the Sloan Digital Sky Surveys: Targeting and First Spectra from SDSS-V (2023, background): “…focused entirely on spectroscopy and comprised an extension of SEGUE (SEGUE2; Rockosi et al. 2022); a radial velocity exoplanet survey (MARVELS; Ge et al. 2008); a clustering survey of galaxies and intergalactic gas in the distant universe (BOSS; Dawson et al. 2013), which required an upgrade…”
The Apache Point Observatory Galactic Evolution Experiment (APOGEE) (2007, unknown): “Such longer fields were not only desired for APOGEE, but they were a necessary part of the observing plan because, initially, APOGEE shared bright time observations with the Multi-Object APO Radial Velocity Exoplanet Large-area Survey (MARVELS) project (Ge et al. 2008; Zhao et al. 2009).”
On the Cool Side: Modeling the Atmospheres of Brown Dwarfs and Giant Planets (2014, background): “Numerous global circulation models (GCMs) for hot Jupiters (see, e.g., review by Showman et al. 2008) and brown dwarfs (Showman & Kaspi 2013; Zhang & Showman 2014) exist.”