Results 131 to 140 of about 398,118 (263)
Breathing Life Into Dead-Zones
The terrestrial planet formation regions of protoplanetary disks are generally sufficiently cold to be con- sidered non-magnetized and, consequently, dynamically inactive.
Gressel Oliver +2 more
doaj +1 more source
The Formation and Dynamics of Super-Earth Planets
Super-Earths, objects slightly larger than Earth and slightly smaller than Uranus, have found a special place in exoplanetary science. As a new class of planetary bodies, these objects have challenged models of planet formation at both ends of the ...
Haghighipour, Nader
core +1 more source
Linking planetesimal and dust content in protoplanetary disks via a local toy model [PDF]
Konstantin Gerbig +2 more
openalex +1 more source
On Kinematic Measurements of Self-gravity in Protoplanetary Disks
Using controlled injection and recovery experiments, we devised an analysis prescription to assess the quality of dynamical measurements of protoplanetary disk gas masses based on resolved (CO) spectral line data, given observational limitations ...
Sean M. Andrews +4 more
doaj +1 more source
The Meteoritical Society: Business from 2023 to 2024
Meteoritics &Planetary Science, Volume 60, Issue 3, Page 680-696, March 2025.
Nancy L. Chabot +2 more
wiley +1 more source
The Carbon Isotopic Ratio and Planet Formation
We 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
doaj +1 more source
Observations of inhomogeneities in protoplanetary disks
In this review I will give a brief overview of the latest observational constraints on the structure and dynamics of protoplanetary disks, with a particular emphasis on the topic of the conference: vortices.
Dullemond Cornelis
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
Observations of edge-on protoplanetary disks with ALMA I. Results from continuum data [PDF]
M. Villenave +17 more
openalex +1 more source
Our understanding of how exoplanets form and evolve relies on analyses of both the mineralogy of protoplanetary disks and their detailed structures; however, these key complementary aspects of disks are usually studied separately.
William Grimble +9 more
doaj +1 more source

