Results 41 to 50 of about 2,101,430 (372)

The Chemical Evolution of the Galaxy: the two-infall model [PDF]

open access: yes, 1996
In this paper we present a new chemical evolution model for the Galaxy which assumes two main infall episodes for the formation of halo-thick disk and thin disk, respectively. We do not try to take into account explicitly the evolution of the halo but we
C.   +5 more
core   +2 more sources

Power scaling of ultrafast oscillators: 350-W average-power sub-picosecond thin-disk laser.

open access: yesOptics Express, 2019
We report a semiconductor saturable absorber mirror (SESAM)-modelocked thin-disk laser oscillator delivering a record 350-W average output power with 940-fs, 39-µJ pulses at 8.88-MHz repetition rate and 37-MW peak power.
F. Saltarelli   +5 more
semanticscholar   +1 more source

Computational Fluid Dynamics Assessment of Flow Characteristic of Thin Liquid Film over Smooth and Corrugated Rotating Disk Surface

open access: yesChemical Engineering Transactions, 2017
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

The Gaia-ESO Survey: Separating disk chemical substructures with cluster models [PDF]

open access: yes, 2015
(Abridged) Recent spectroscopic surveys have begun to explore the Galactic disk system outside the solar neighborhood on the basis of large data samples.
Alfaro, E. J.   +26 more
core   +4 more sources

Femtosecond Yb:CaGdAlO_4 thin-disk oscillator [PDF]

open access: yesOptics Letters, 2012
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

Isotopic Titanium Abundances in Local M Dwarfs [PDF]

open access: yes, 2009
Relative abundances of the five stable isotopes of titanium (^46Ti to ^50Ti) are measured for 11 M dwarfs belonging to the thin disk (four stars), thick disk (three stars), the halo (one star), and either the thick or the thin disk (three stars).
Asplund   +30 more
core   +2 more sources

Turbulent convection in thin accretion disks [PDF]

open access: yesThe Astrophysical Journal, 1995
38 pages including 1 PostScript ...
Itzhak Goldman, Amri Wandel
openaire   +4 more sources

Thin accretion disk around a four-dimensional Einstein-Gauss-Bonnet black hole [PDF]

open access: yesChinese Physics C, High Energy Physics & Nuclear Physics, 2020
Recently, a novel four-dimensional Einstein-Gauss-Bonnet (4EGB) theory of gravity was proposed by Glavan and Lin [D. Glavan and C. Lin, Phys. Rev. Lett.
C. Liu 刘, T. Zhu 朱, Qiang 强 Wu 武
semanticscholar   +1 more source

Ultrafast thin disk lasers: sub-100 fs pulse duration and carrier envelope offset detection

open access: yesEPJ Web of Conferences, 2013
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

Stochastic processes, galactic star formation, and chemical evolution. Effects of accretion, stripping, and collisions in multiphase multi-zone models [PDF]

open access: yes, 2005
This paper reports simulations allowing for stochastic accretion and mass loss within closed and open systems modeled using a previously developed multi-population, multi-zone (halo, thick disk, thin disk) treatment.
Casuso   +35 more
core   +2 more sources

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