Results 201 to 210 of about 16,853 (286)
Formation of terrestrial planets from planetesimals around M dwarfs [PDF]
Masahiro Ogihara, Shigeru Ida
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From Grains to Planetesimals: Les Houches Lecture [PDF]
Andrew N. Youdin
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The convective overstability (COS) is a hydrodynamic instability occurring in protoplanetary disk (PPD) regions with an adverse radial entropy gradient. It is a potential driver of turbulence and may influence planetesimal formation. In this second paper
Marius Lehmann, Min-Kai Lin
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A pebble accretion model for the formation of the terrestrial planets in the Solar System. [PDF]
Johansen A+6 more
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Planetesimal Evolution in Circumbinary Gaseous Disks: A Hybrid Model [PDF]
F. Marzari, P. Thébault, H. Schöll
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Terrestrial planet and asteroid belt formation by Jupiter-Saturn chaotic excitation. [PDF]
Lykawka PS, Ito T.
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From planetesimals to terrestrial planets: N-body simulations including the effects of nebular gas and giant planets [PDF]
R. Morishima, Joachim Stadel, Ben Moore
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On the origin and evolution of the asteroid Ryugu: A comprehensive geochemical perspective. [PDF]
Nakamura E+89 more
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Accretion rates of planetesimals by protoplanets embedded in nebular gas [PDF]
Takayuki Tanigawa, Keiji Ohtsuki
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