Results 131 to 140 of about 394,629 (288)
Magma Ocean Evolution at Arbitrary Redox State
Abstract Interactions between magma oceans and overlying atmospheres on young rocky planets leads to an evolving feedback of outgassing, greenhouse forcing, and mantle melt fraction. Previous studies have predominantly focused on the solidification of oxidized Earth‐similar planets, but the diversity in mean density and irradiation observed in the low ...
Harrison Nicholls+3 more
wiley +1 more source
Exploring the Complex Ionization Environment of the Turbulent DM Tau Disk
Ionization drives important chemical and dynamical processes within protoplanetary disks, including the formation of organics and water in the cold midplane and the transportation of material via accretion and magnetohydrodynamic flows.
Deryl E. Long+11 more
doaj +1 more source
Formation and evolution of the protoplanetary disk [PDF]
A disk formation model during collapse of the protosolar nebula, yielding a low-mass protoplanetary disk is presented. The following subject areas are covered: (1) circumstellar disks; (2) conditions for the formation of stars with disks; (3) early ...
Makalkin, A. B., Ruzmaikina, Tamara V.
core +1 more source
Protoplanetary Disk Resonances and Type I Migration [PDF]
Waves reflected by the inner edge of a protoplanetary disk are shown to significantly modify Type I migration, even allowing the trapping of planets near the inner disk edge for small planets in a range of disk parameters.
Abramowitz+16 more
core +2 more sources
The Evidence of Radio Polarization Induced by the Radiative Grain Alignment and Self-scattering of Dust Grains in a Protoplanetary Disk [PDF]
The mechanisms causing millimeter-wave polarization in protoplanetary disks are under debate. To disentangle the polarization mechanisms, we observe the protoplanetary disk around HL Tau at 3.1 mm with the Atacama Large Millimeter/submillimeter Array ...
A. Kataoka+7 more
semanticscholar +1 more source
Resonant Relaxation in Protoplanetary Disks [PDF]
19 pages, 1 figure, LaTeX, submitted to ...
openaire +3 more sources
FIRST DETECTION OF GAS-PHASE METHANOL IN A PROTOPLANETARY DISK [PDF]
The first detection of gas-phase methanol in a protoplanetary disk (TW Hya) is presented. In addition to being one of the largest molecules detected in disks to date, methanol is also the first disk organic molecule with an unambiguous ice chemistry ...
C. Walsh+9 more
semanticscholar +1 more source
Differences in elemental abundances between CI chondrites and the solar photosphere
Abstract CI chondrites have been a proxy for the solar system since the mid‐20th century. The photospheric and CI chondrite abundances (P and CI, respectively) show a strong correlation. CI as a proxy is also justified by the (i) smoothness of their abundances plotted as a function of odd mass number and (ii) agreement within the error of P as ...
A. J. G. Jurewicz+3 more
wiley +1 more source
The Determination of Protoplanetary Disk Masses [PDF]
In this article we review the methods used to determine the gas and dust masses of protoplanetary disks, with an emphasis on the lesser characterized total gas mass. Our review encompasses all the indirect tracers and the methodology that is be used to isolate the hidden H2 via dust, CO, and HD emission.
Jonathan P. Williams, Edwin A. Bergin
openaire +3 more sources
A Deep Search for Complex Organic Molecules toward the Protoplanetary Disk of V883 Ori
Complex organic molecules (COMs) in the form of prebiotic molecules are potential building blocks of life. Using Atacama Large Millimeter/submillimeter Array Band 7 observations in spectral scanning mode, we carried out a deep search for COMs within the ...
Abubakar M. A. Fadul+6 more
doaj +1 more source