Results 31 to 40 of about 282,866 (344)
Thick disk kinematics from RAVE and the solar motion [PDF]
Radial velocity surveys such as the Radial Velocity Experiment (RAVE) provide us with measurements of hundreds of thousands of nearby stars most of which belong to the Galactic thin, thick disk or halo. Ideally, to study the Galactic disks (both thin and
A. Silviero +125 more
core +2 more sources
Abundance trends in the thin and thick disks [PDF]
Review article presented at the ESO-ARCETRI workshop on: Chemical Abundances and Mixing in Stars in the Milky Way and its Satellites (September 13-17 2004), To be published in "ESO Astrophysics Symposia", Editors: Luca Pasquini and Sofia Randich, 6 pages, 4 figures (one in colour)
S. Feltzing
openalex +5 more sources
Process Intensification (PI) is used for analysis and design of innovative equipment and processing methods with substantially improved sustainability, efficiency and environmental performance.
P. Suppramaniam +3 more
doaj +1 more source
Treating gravity in thin-disk simulations [PDF]
13 pages, 19 figures, accepted for publication in A& ...
Farzana Meru +3 more
openaire +4 more sources
Ultrafast thin disk lasers: sub-100 fs pulse duration and carrier envelope offset detection
We present two milestone results that confirm that thin disk lasers are excellent candidates for driving extreme nonlinear optics experiments. In a first experiment using the broadband mixed sesquioxide gain material Yb:LuScO3, we demonstrate that thin ...
Huber Günter +10 more
doaj +1 more source
The Geneva-Copenhagen Survey of the Solar neighbourhood II. New uvby calibrations and rediscussion of stellar ages, the G dwarf problem, age-metallicity diagram, and heating mechanisms of the disk [PDF]
Ages, metallicities, space velocities, and Galactic orbits of stars in the Solar neighbourhood are fundamental observational constraints on models of galactic disk evolution.
Allende Prieto +56 more
core +1 more source
Femtosecond Yb:CaGdAlO_4 thin-disk oscillator [PDF]
A mode-locked thin-disk laser based on Yb:CALGO is demonstrated for the first time. At an average output power of 28 W we obtained pulses with a duration of 300 fs and a pulse energy of 1.3 μJ. 197 fs pulses with 0.9 μJ of energy were achieved at an average output power of 20 W.
Ricaud, Sandrine +14 more
openaire +4 more sources
We experimentally investigate the settling of millimetre-sized thin disks in quiescent air. The range of physical parameters is chosen to be relevant to plate crystals settling in the atmosphere: the diameter-to-thickness aspect ratio is$\chi =25\unicode{x2013}60$, the Reynolds numbers based on the disk diameter and fall speed are$Re=O(10^2)$and the ...
Amy Tinklenberg +2 more
openaire +1 more source
The Relative Age of the Thin and Thick Galactic Disks [PDF]
We determine the relative ages of the open cluster NGC 188 and selected Hipparcos field stars by isochrone fitting, and compare them to the age of the thick disk globular cluster 47 Tuc. The best fit age for NGC 188 was determined to be $6.5 \pm 1.0$ Gyr.
Brian Chaboyer +7 more
core +4 more sources
Turbulent convection in thin accretion disks [PDF]
38 pages including 1 PostScript ...
Itzhak Goldman, Amri Wandel
openaire +4 more sources

