Radial Migration of Planetesimals

1994 ◽  
pp. 49-56
Author(s):  
R. Neuhäuser ◽  
J. V. Feitzinger
Keyword(s):  
Radial Migration

Two modes of radial migration in early development of the cerebral cortex

10.1038/83967 ◽  
2001 ◽  
Vol 4 (2) ◽  
pp. 143-150 ◽  
Author(s):  
Bagirathy Nadarajah ◽  
Janice E. Brunstrom ◽  
Jaime Grutzendler ◽  
Rachel O. L. Wong ◽  
Alan L. Pearlman
Keyword(s):  
Cerebral Cortex ◽  
Early Development ◽  
Radial Migration

scholarly journals Radial Migration Dynamics Is Modulated in a Laminar and Area-Specific Manner During Primate Corticogenesis

2020 ◽  
Vol 8 ◽  
Author(s):  
Veronique Cortay ◽  
Delphine Delaunay ◽  
Dorothée Patti ◽  
Elodie Gautier ◽  
Nathalie Doerflinger ◽  
...  
Keyword(s):  
Radial Migration ◽  
Specific Manner ◽  
Migration Dynamics

scholarly journals Galaxy Dynamics: Secular Evolution and Accretion

2010 ◽  
Vol 6 (S271) ◽  
pp. 119-126 ◽  
Author(s):  
Francoise Combes
Keyword(s):  
Angular Momentum ◽  
Galaxy Evolution ◽  
Resonant Scattering ◽  
Relative Role ◽  
Radial Migration ◽  
Galaxy Dynamics ◽  
Secular Evolution ◽  
Minor Mergers ◽  
Gas Accretion

AbstractRecent results are reviewed on galaxy dynamics, bar evolution, destruction and re-formation, cold gas accretion, gas radial flows and AGN fueling, minor mergers. Some problems of galaxy evolution are discussed in particular, exchange of angular momentum, radial migration through resonant scattering, and consequences on abundance gradients, the frequency of bulgeless galaxies, and the relative role of secular evolution and hierarchical formation.

scholarly journals Shaping Disk Galaxy Stellar Populations via Internal and External Processes

2012 ◽  
Vol 10 (H16) ◽  
pp. 372-372
Author(s):  
Rok Roškar
Keyword(s):  
Galaxy Formation ◽  
Stellar Population ◽  
Milky Way ◽  
Stellar Populations ◽  
Radial Migration ◽  
Disk Formation ◽  
Process Understanding ◽  
History Of ◽  
Nearby Galaxies ◽  
Gas Accretion

AbstractIn recent years, effects such as the radial migration of stars in disks have been recognized as important drivers of the properties of stellar populations. Radial migration arises due to perturbative effects of disk structures such as bars and spiral arms, and can deposit stars formed in disks to regions far from their birthplaces. Migrant stars can significantly affect the demographics of their new locales, especially in low-density regions such as in the outer disks. However, in the cosmological environment, other effects such as mergers and filamentary gas accretion also influence the disk formation process. Understanding the relative importance of these processes on the detailed evolution of stellar population signatures is crucial for reconstructing the history of the Milky Way and other nearby galaxies. In the Milky Way disk in particular, the formation of the thickened component has recently attracted much attention due to its potential to serve as a diagnostic of the galaxy's early history. Some recent work suggests, however, that the vertical structure of Milky Way stellar populations is consistent with models that build up the thickened component through migration. I discuss these developments in the context of cosmological galaxy formation.

scholarly journals BMP signaling and radial migration of cortical neurons

2017 ◽  
Vol 145 ◽  
pp. S115
Author(s):  
Nitin Agnihotri ◽  
Monika Saxena ◽  
Jonaki Sen
Keyword(s):  
Cortical Neurons ◽  
Bmp Signaling ◽  
Radial Migration

scholarly journals Signatures of radial migration in barred galaxies: Azimuthal variations in the metallicity distribution of old stars

2013 ◽  
Vol 553 ◽  
pp. A102 ◽  
Author(s):  
P. Di Matteo ◽  
M. Haywood ◽  
F. Combes ◽  
B. Semelin ◽  
O. N. Snaith
Keyword(s):  
Radial Migration ◽  
Barred Galaxies ◽  
Metallicity Distribution
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