Works matching IS 17439213 AND DT 2007 AND VI 3 AND IP S249
Results: 77
Dynamics and instabilities in exoplanetary systems.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 441, doi. 10.1017/S1743921308016955
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Orbital determination and dynamics of resonant extrasolar planetary systems.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 427, doi. 10.1017/S1743921308016943
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Effects of dissipating gas drag on planetesimal accretion in binary systems.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 419, doi. 10.1017/S1743921308016931
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Origin of debris disks and the supply of metals in DZ white dwarfs.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 389, doi. 10.1017/S1743921308016876
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Baroclinic generation of potential vorticity in an embedded planet-disk system.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 407, doi. 10.1017/S1743921308016918
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Retrograde resonances in compact multi-planetary systems: a feasible stabilizing mechanism.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 511, doi. 10.1017/S1743921308017055
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Orbital stability of planets in binary systems: A new look at old results.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 507, doi. 10.1017/S1743921308017043
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Habitability of super-Earths: Gliese 581c & 581d.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 503, doi. 10.1017/S1743921308017031
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Habitable zones for Earth-mass planets in multiple planetary systems.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 499, doi. 10.1017/S174392130801702X
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Analysis of near-separatrix motion in planetary systems.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 491, doi. 10.1017/S1743921308017018
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Formation and transformation of the 3:1 mean-motion resonance in 55 Cancri System.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 485, doi. 10.1017/S1743921308017006
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Secular evolution of exoplanetary systems and close encounters.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 479, doi. 10.1017/S1743921308016992
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Extrasolar planet interactions.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 469, doi. 10.1017/S1743921308016980
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On the dynamics of Trojan planets in extrasolar planetary systems.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 461, doi. 10.1017/S1743921308016979
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Stability constraints in modeling of multi-planet extrasolar systems.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 447, doi. 10.1017/S1743921308016967
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The effect of poloidal magnetic field on type I planetary migration.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 401, doi. 10.1017/S1743921308016906
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On type I planetary migration in adiabatic disks.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 397, doi. 10.1017/S174392130801689X
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Type I planetary migration in a self-gravitating disk.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 393, doi. 10.1017/S1743921308016888
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Runaway migration in a multiple-protoplanet system.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 413, doi. 10.1017/S174392130801692X
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3D SPH simulations of grain growth in protoplanetary disks.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 385, doi. 10.1017/S1743921308016864
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Origin of the dusty disks around white dwarfs.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 381, doi. 10.1017/S1743921308016852
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Dust evolution in protoplanetary disks.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 375, doi. 10.1017/S1743921308016840
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Astromineralogy of protoplanetary disks.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 369, doi. 10.1017/S1743921308016839
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Searching for H2 emission from protoplanetary disks using near- and mid-infrared high-resolution spectroscopy.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 359, doi. 10.1017/S1743921308016827
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Disc signatures in a new population of low mass YSOs in ρ Ophiuchi.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 355, doi. 10.1017/S1743921308016815
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On the solar system—debris disk connection.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 347, doi. 10.1017/S1743921308016803
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Planetary migration in gaseous protoplanetary disks.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 331, doi. 10.1017/S1743921308016797
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On the formation age of the first planetary system.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 325, doi. 10.1017/S1743921308016785
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Habitable planet formation in extreme planetary systems: systems with multiple stars and/or multiple planets.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 319, doi. 10.1017/S1743921308016773
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Formation and detectability of Earth-like planets around Alpha-Centauri B.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 313, doi. 10.1017/S1743921308016761
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Retention of protoplanetary cores near the snowline.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 309, doi. 10.1017/S174392130801675X
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Formation of terrestrial planets from planetesimals around M dwarfs.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 305, doi. 10.1017/S1743921308016748
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Giant impact, planetary merger, and diversity of planetary-core mass.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 301, doi. 10.1017/S1743921308016736
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Planet formation around intermediate mass stars.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 293, doi. 10.1017/S1743921308016724
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Migration and Final Location of Hot Super Earths in the Presence of Gas Giants.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 285, doi. 10.1017/S1743921308016712
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The formation of close-in planets by the slingshot model.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 279, doi. 10.1017/S1743921308016700
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SPH simulations of star/planet formation triggered by cloud-cloud collisions.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 271, doi. 10.1017/S1743921308016694
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Formation of heavy element rich giant planets by giant impacts.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 267, doi. 10.1017/S1743921308016682
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Tidal barrier and the asymptotic mass of proto gas-giant planets.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 263, doi. 10.1017/S1743921308016670
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Observational tests of planet formation models.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 261, doi. 10.1017/S1743921308016669
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Planet formation in binary stars.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 251, doi. 10.1017/S1743921308016657
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Terrestrial planet formation in extra-solar planetary systems.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 233, doi. 10.1017/S1743921308016645
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Orbital migration and mass-semimajor axis distributions of extrasolar planets.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 223, doi. 10.1017/S1743921308016633
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Testing planet formation theories with giant stars.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 209, doi. 10.1017/S1743921308016621
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Tidal evolution of close-in extra-solar planets.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 187, doi. 10.1017/S1743921308016591
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Modeling of evolution of the rotational axis of “hot Jupiter” planets under tidal perturbations.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 197, doi. 10.1017/S1743921308016608
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Astrobiological effects of F, G, K and M main-sequence stars.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 203, doi. 10.1017/S174392130801661X
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Finding new sub-stellar co-moving companion candidates - the case of CT Cha.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 65, doi. 10.1017/S1743921308016396
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Tidal friction in close-in planets.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 179, doi. 10.1017/S174392130801658X
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Preparing the exoplanet search with PRIMA: searching for reference stars and target characterization.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S249, p. 61, doi. 10.1017/S1743921308016384
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