Vorticity‐induced Wave Motion in a Compressible Protoplanetary Disk [PDF]
, 2002 S. S. Davis
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UniverseGravitational fragmentation of a protoplanetary disk is considered a possible mechanism for the formation of planets and brown dwarfs. In this process, transitory objects are formed that are known as clumps, which are compact gas–dust condensations with ...
Eduard Vorobyov, Carina Schoenhacker
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Isotopic evolution of the protoplanetary disk and the building blocks of Earth and the Moon. [PDF]
Nature, 2018 Schiller M, Bizzarro M, Fernandes VA.
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Evidence for a Developing Gap in a 10 Myr Old Protoplanetary Disk [PDF]
, 2002 Nuria Calvet +5 more
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The Carbon Isotopic Ratio and Planet Formation
The Astrophysical JournalWe present the first detection of ^13 CCH in a protoplanetary disk (TW Hya). Using observations of C _2 H, we measure CCH/ ^13 CCH = 65 ± 20 gas with a CO isotopic ratio of ^12 CO/ ^13 CO = 21 ± 5.
Edwin A. Bergin +8 more
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Chondrules as direct thermochemical sensors of solar protoplanetary disk gas. [PDF]
Sci Adv, 2018 Libourel G, Portail M.
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Igneous processes in the small bodies of the Solar System I. Asteroids and comets. [PDF]
iScience, 2023 Leone G, Tanaka HKM.
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Formation of Giant Planets by Fragmentation of Protoplanetary Disks [PDF]
, 2002 Lucio Mayer +3 more
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The background temperature of the protoplanetary disk within the first four million years of the Solar System. [PDF]
Earth Planet Sci Lett, 2018 Schrader DL +3 more
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Investigation of the Physical Properties of Protoplanetary Disks around T Tauri Stars by a 1 Arcsecond Imaging Survey: Evolution and Diversity of the Disks in Their Accretion Stage [PDF]
, 2002 Yoshimi Kitamura +5 more
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