Results 61 to 70 of about 221,035 (206)
Spectrophotometrically Identified stars in the PEARS-N and PEARS-S fields [PDF]
Deep ACS slitless grism observations and identification of stellar sources are presented within the Great Observatories Origins Deep Survey (GOODS) North and South fields which were obtained in the Probing Evolution And Reionization Spectroscopically ...
A. J. Burgasser +28 more
core +3 more sources
Disk-Halo Interaction - I. Three-Dimensional Evolution of the Galactic Disk
The results of a three-dimensional model for disk-halo interaction are presented here. The model considers explicitly the input of energy and mass by isolated a nd correlated supernovae in the disk.
de Avillez, Miguel A.
core +2 more sources
Thin disk kinematics from RAVE and the solar motion [PDF]
Aims. We study the Milky Way thin disk with the Radial Velocity Experiment (RAVE) survey. We consider the thin and thick disks as different Galactic components and present a technique to statistically disentangle the two populations.
Bertelli, G. +16 more
core +2 more sources
Using disk form multilayers, a semi-analytical solution has been derived for determination of displacements and stresses in a rotating cylindrical shell with variable thickness under uniform pressure.
Mohammad Zamani Nejad +2 more
doaj +1 more source
Impacts of Radial Mixing on the Galactic Thick and Thin Disks
Using N-body simulations of the Galactic disks, we qualitatively study how the metallicity distributions of the thick and thin disk stars are modified by radial mixing induced by the bar and spiral arms.
Kawata, Daisuke
core +1 more source
We analyze high quality abundances data of solar neighborhood stars and show that there are two distinct regimes of [alpha/Fe] versus age which we identify as the epochs of the thick and thin disk formation.
Di Matteo, P. +4 more
core +2 more sources
Atacama Large Millimeter Array (ALMA) surveys have suggested that the dust in Class II disks may not be enough to explain the averaged solid mass in exoplanets, under the assumption that the mm disk continuum emission is optically thin.
Andrews, Sean M. +12 more
core +2 more sources
Unveiling the Structure of Pre-Transitional Disks
In the past few years, several disks with inner holes that are empty of small dust grains have been detected and are known as transitional disks. Recently, Spitzer has identified a new class of "pre-transitional disks" with gaps; these objects have an ...
Andrews +69 more
core +1 more source
(Abridged) We perform an analysis of spectra and photometry for 22,770 stars included in the third data release (DR3) of the SDSS. We measure radial velocities and, based on a model-atmosphere analysis, derive estimates ofthe atmospheric parameters ...
Alongi M. +20 more
core +2 more sources
The Evolution of the Optically Thick Accretion Disk in Nova Muscae [PDF]
Ranjeev Misra, Fulvio Melia
openalex +1 more source

