Suggested Topics within your search.
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Doppler imaging
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Evaporation
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Grain size and shape
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Jupiter
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Jupiters
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Planet and satellite: gaseous planet
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Planet-disk interactions
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Planet-star interactions
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Planets
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Planets and satellites
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Planets and satellites: detections
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Population synthesis
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Protoplanetary disks
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Satellites
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Solar System dynamics
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Stability of Mercury
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Stars
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Stellar cluster
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Stellars
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Symplectic methods
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astronomical instrumentation
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hydrodynamics
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planet-disc interactions
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planet-star interactions
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planetary science
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planets and satellites: detections
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planets and satellites: gaseous planets
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protoplanetary discs
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telescopes
1
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181by K. A. Radchenko“... retrograde satellites of giant planets known to date, meet the criteria for persistence of Lagrange...”
Published 2013-10-01
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182by Wittenmyer, Robert Andrew, 1976-“... planets in any of these 22 systems, despite dynamical feasibility. The frequency of inner giant planets...”
Published 2012
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183by Narayanan, Desika T“... giant planets and galaxies. The main results of this thesis follow. (1) Gas giant protoplanets may...”
Published 2007
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185by Čelebonović V.“... equilibrium in a LJ fluid. Interesting kinds of such systems are the giant planets and the icy satellites...”
Published 2010-01-01
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186by Celebonovic, V.“... kinds of such systems are the giant planets and the icy satellites in various planetary systems...”
Published 2010-12-01
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187by Guenel, Mathieu“... the Sun (i.e. from M- to F-type stars), as well as in Jupiter- and Saturn-like gaseous giant planets. We...”
Published 2016
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188by Pena, Fernando Gabriel“...Many known extra-solar giant planets lie close to their host stars. Around 60 have their semi-major...”
Published 2010
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189by Pena, Fernando Gabriel“...Many known extra-solar giant planets lie close to their host stars. Around 60 have their semi-major...”
Published 2010
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190by Kao, Melodie Minyu“...<p>Brown dwarfs share characteristics with both low-mass stars and gas giant planets, making them...”
Published 2017
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191by Robertson, Paul Montgomery“... and the presence of giant planets, but also reveals a significant metallicity dependence on the presence of high...”
Published 2010
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192by Valenti Jeff A.“... be selected wisely. For giant planets, it is now well established that stars with higher metallicity are more...”
Published 2013-04-01
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193by Yu. Kuznyetsova, A. Vidmachenko, O. Matsiaka, Y. Shliakhetskaya, M. Yushkin, V. Krushevska“...The results of long-term spectral observations of Solar System giant planets Uranus and Neptune...”
Published 2016-06-01
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194by Sozzetti A.“...In its all-sky astrometric survey, Gaia will be sensitive to giant planets orbiting within a few...”
Published 2013-04-01
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195by Lin Min-Kai“...Numerical simulations are presented to study the stability of gaps opened by giant planets in 3D...”
Published 2013-04-01
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196“..., and at the Alfvén radius in the equatorial magnetosphere of rapidly rotating strongly magnetized giant planets...”
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197by Raymond Sean“... reproduced. As the giant planets migrate back outward they re-populate the asteroid belt from two different...”
Published 2014-02-01
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198by Brucalassi, Anna“... at the Wendelstein Observatory, and the search of giant planets around stars in the open cluster Messier-67 (M67...”
Published 2014
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199“... of less massive giant planets (< 1 Jupiter mass) within 0.035AU from their parent stars. We employ...”
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