Isotopic evolution of the protoplanetary disk and the building blocks of Earth and the Moon. [PDF]
Schiller M, Bizzarro M, Fernandes VA.
europepmc +1 more source
One of the most active fields of research in accretion disk theory is understanding the mechanisms that transport angular momentum outward. Two instabilities are thought to be responsible for it in massive, magnetized disks: the magnetorotational instability (MRI) caused by the presence of a weak magnetic field, and gravitational instabilities.This PhD
openaire +1 more source
We analyze near-infrared integral field spectropolarimetry of the AB Aurigae protoplanetary disk and protoplanet (AB Aur b), obtained with SCExAO/CHARIS in 22 wavelength channels covering the J , H , and K passbands ( λ _0 = 1.1–2.4 μ m) over angular ...
Erica Dykes +23 more
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Chondrules as direct thermochemical sensors of solar protoplanetary disk gas. [PDF]
Libourel G, Portail M.
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Magnetic disk winds in protoplanetary disks: Description of the model and impact on global disk evolution [PDF]
Kundan Kadam +4 more
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Light Echoes of Protoplanetary Disks
Light echoes offer a means of studying protoplanetary disks, including their geometry and composition, even when they are not spatially resolved. We present a test of this approach applied specifically to optically thick, geometrically flared disks ...
Austin J. King, Benjamin C. Bromley
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The background temperature of the protoplanetary disk within the first four million years of the Solar System. [PDF]
Schrader DL +3 more
europepmc +1 more source
Coordinated Space- and Ground-based Monitoring of Accretion Bursts in a Protoplanetary Disk: The Orbital and Accretion Properties of DQ Tau [PDF]
Hala Alqubelat +11 more
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Probing midplane CO abundance and gas temperature with DCO+in the protoplanetary disk around HD 169142 [PDF]
M. T. Carney +10 more
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A new method for direct measurement of isotopologue ratios in protoplanetary disks: a case study of the $^{12}$CO/$^{13}$CO ratio in the TW Hya disk [PDF]
Tomohiro C. Yoshida +4 more
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