1,550,382 research outputs found
The oxygen vs. sodium (anti)correlation(s) in omega Cen
Recent exam of large samples of omega Cen giants shows that it shares with
mono-metallic globular clusters the presence of the sodium versus oxygen
anticorrelation, within each subset of stars with iron content in the range
-1.9<~[Fe/H]<~-1.3. These findings suggest that, while the second generation
formation history in omega Cen is more complex than that of mono-metallic
clusters, it shares some key steps with those simpler cluster. In addition, the
giants in the range -1.3<[Fe/H]<~-0.7 show a direct O--Na correlation, at
moderately low O, but Na up to 20 times solar. These peculiar Na abundances are
not shared by stars in other environments often assumed to undergo a similar
chemical evolution, such as in the field of the Sagittarius dwarf galaxy. These
O and Na abundances match well the yields of the massive asymptotic giant
branch stars (AGB) in the same range of metallicity, suggesting that the stars
at [Fe/H]>-1.3 in omega Cen are likely to have formed directly from the pure
ejecta of massive AGBs of the same metallicities. This is possible if the
massive AGBs of [Fe/H]>-1.3 in the progenitor system evolve when all the
pristine gas surrounding the cluster has been exhausted by the previous star
formation events, or the proto--cluster interaction with the Galaxy caused the
loss of a significant fraction of its mass, or of its dark matter halo, and the
supernova ejecta have been able to clear the gas out of the system. The absence
of dilution in the metal richer populations lends further support to a scenario
of the formation of second generation stars in cooling flows from massive AGB
progenitors. We suggest that the entire formation of omega Cen took place in a
few 10^8yr, and discuss the problem of a prompt formation of s--process
elements.Comment: The Astrophysical Journal, in pres
From the fuzzy disc to edge currents in Chern-Simons Theory
We present a brief review of the fuzzy disc, the finite algebra approximating
functions on a disc, which we have introduced earlier. We also present a
comparison with recent papers of Balachandran, Gupta and
K\"urk\c{c}\"{u}o\v{g}lu, and of Pinzul and Stern, aimed at the discussion of
edge states of a Chern-Simons theory.Comment: 8 pages, 6 figures, Talk presented at ``Space-time and Fundamental
Interactions: Quantum Aspects'', conference in honour of A. P. Balachandran's
65th birthday. References added and one misprint correcte
Optical and X-ray Properties of CAL 83: I. Quasi-periodic Optical and Supersoft Variability
We have studied the long-term (~ years) temporal variability of the prototype
supersoft X-ray source (SSS) CAL 83 in the LMC, using data from the MACHO and
OGLE projects. The CAL 83 light curve exhibits dramatic brightness changes of
~1 mag on timescales of ~450 days, and spends typically ~200 days in the
optical low state. Combined with archival XMM-Newton X-ray observations these
represent the most extensive X-ray/optical study to date of this system, and
reveal in much greater detail that the X-ray light curve is anti-correlated
with the optical behaviour. This is remarkably similar to the behaviour of the
"transient" SSS, RX J0513.9-6951, where the SSS outbursts recur on a timescale
of ~168 days, and also anti-correlate with the optical flux. We performed
simple blackbody fits to both high and low state X-ray spectra, and find that
the blackbody temperature and luminosity decrease when the optical counterpart
brightens. We interpret these long-term variations in terms of the limit-cycle
model of Hachisu & Kato (2003a), which provides further support for these
systems containing massive (~1.3 Msun) white dwarfs. In addition, we have
refined their orbital periods in the MACHO and OGLE-III light curves to values
of 1.047529(1) days and 0.762956(5) days for CAL 83 and RX J0513.9-6951,
respectively.Comment: 9 pages, 8 figures, 3 tables, accepted for publication in MNRA
Coherence scale of the two-dimensional Kondo Lattice model
A doped hole in the two-dimensional half-filled Kondo lattice model with
exchange J and hopping t has momentum (pi,pi) irrespective of the coupling J/t.
The quasiparticle residue of the doped hole, Z_{(\pi, \pi)}, tracks the Kondo
scale, T_K, of the corresponding single impurity model. Those results stem from
high precision quantum Monte Carlo simulations on lattices up to 12 X 12.
Accounting for small dopings away from half-filling within a rigid band
approximation, this result implies that the effective mass of the charge
carriers at the Fermi level tracks 1/T_K or equivalently that the coherence
temperature T_{coh} \propto T_K. This results is consistent with the large-N
saddle point of the SU(N) symmetric Kondo lattice model.Comment: 4 pages, 4 figure
Longitudinal and Transverse Form Factors from C
Electron scattering form factors from C have been studied in the
framework of the particle-hole shell model. Higher configurations are taken
into account by allowing particle-hole excitations from the 1 and 1
shells core orbits up to the 1 shell. The inclusion of the higher
configurations modifies the form factors markedly and describes the
experimental data very well in all momentum transfer regions.Comment: 5 pages, 5 figures, 3 tables, late
A unique model for the variety of multiple populations formation(s) in globular clusters: a temporal sequence
We explain the multiple populations recently found in the 'prototype'
Globular Cluster (GC) NGC 2808 in the framework of the asymptotic giant branch
(AGB) scenario. The chemistry of the five -or more- populations is
approximately consistent with a sequence of star formation events, starting
after the supernovae type II epoch, lasting approximately until the time when
the third dredge up affects the AGB evolution (age ~90-120Myr), and ending when
the type Ia supernovae begin exploding in the cluster, eventually clearing it
from the gas. The formation of the different populations requires episodes of
star formation in AGB gas diluted with different amounts of pristine gas. In
the nitrogen-rich, helium-normal population identified in NGC 2808 by the UV
Legacy Survey of GCs, the nitrogen increase is due to the third dredge up in
the smallest mass AGB ejecta involved in the star formation of this population.
The possibly-iron-rich small population in NGC 2808 may be a result of
contamination by a single type Ia supernova. The NGC 2808 case is used to build
a general framework to understand the variety of 'second generation' stars
observed in GCs. Cluster-to-cluster variations are ascribed to differences in
the effects of the many processes and gas sources which may be involved in the
formation of the second generation. We discuss an evolutionary scheme, based on
pollution by delayed type II supernovae, which accounts for the properties of
s-Fe-anomalous clusters.Comment: 20 pages, 7 figures, in press on MNRA
Asymptotics of the deuteron form factors in the nucleon model and JLab experiments
Using the instant form dynamics of Poincar\'e invariant quantum mechanics and
the modified relativistic impulse approximation proposed previously we
calculate asymptotics of electromagnetic form factors for the deuteron
considered as two--nucleon system. We show that today experiment on the elastic
-scattering has reached asymptotic regime. The possible range of momentum
transfer when the quark degrees of freedom could be seen in future JLab
experiments is estimated. The explicit relation between the behavior of
deuteron wave function at and the form factors asymptotics is obtained.
The conditions on wave functions to give the asymptotics predicted by QCD and
quark counting rules are formulated.Comment: 9 pages, 1 figur
RF-MEMS Switched Varactors for Medium Power Applications
In RF (Radio Frequency) domain, one of the limitations of using MEMS (Micro
Electromechanical Systems) switching devices for medium power applications is
RF power. Failure phenomena appear even for 500 mW. A design of MEMS switched
capacitors with an enhanced topology is presented in this paper to prevent it.
This kind of device and its promising performances will serve to fabricate a
MEMS based phase shifter able to work under several watts.Comment: Submitted on behalf of EDA Publishing Association
(http://irevues.inist.fr/handle/2042/16838
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