Automated spectral extraction for high multiplexing MOS and IFU observations
VIMOS main distinguishing characteristic is its very high multiplex capability: in MOS mode up to 800 spectra can be acquired
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Binary Evolution and Neutron Stars in Globular Clusters
We investigate the dynamical formation and evolution of binaries containing neutron stars in dense globular clusters. Our numerical simulations combine
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Can the Red Shift be a consequence of the Dilaton field?
The possibility that the expansion rate of the Universe, as reflected by the Red Shift, could be produced by the
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Chandra, GLAST, and the Galactic Center
Two-temperature spherical accretion flows produce $\approx 100$ Mev gamma-rays from the decay of neutral pions created in proton-proton collisions close
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Characterizing the structure of interstellar turbulence
Modeling the structure of molecular clouds depends on good methods to statistically compare simulations with observations in order to constrain
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COBE, Inflation, and Light Scalars
Comparison of theobservedanisotropy with that predicted iadiabaticDM models suggest that much of thserved signal may be due to long wavelenh
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Collapsars, Gamma-Ray Bursts, and Supernovae
A diverse range of phenomena is possible when a black hole experiences very rapid accretion from a disk due to
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Collider Implications of Kaluza-Klein Excitations of the Electroweak Gauge Bosons
It is possible for the SM fields to propagate into one or more large extra compact dimensions. Such fields have
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Comparison of the energy histograms and conformations between different models of copolymers on lattice
Based on large-scale Monte Carlo simulations on lattice the energy probability distribution functions are investigated for a large set of
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Cooperative Game Theory within Multi-Agent Systems for Systems Scheduling
Research concerning organization and coordination within multi-agent systems continues to draw from a variety of architectures and methodologies. The work
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Development of a carbon fibre composite active mirror: Design and testing
Carbon fibre composite technology for lightweight mirrors is gaining increasing interest in the space- and ground-based astronomical communities for its
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Differentially rotating magnetised neutron stars: production of toroidal magnetic fields
We initiate numerical studies of differentially rotating magnetised (proto) neutron stars by studying - through construction from first principles -
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Duplication Models for Biological Networks
Are biological networks different from other large complex networks? Both large biological and non-biological networks exhibit power-law graphs (number of
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Dust Properties and Assembly of Large Particles in Protoplanetary Disks
Recent research on the buildup of rocks from small dust grains has reaffirmed that grain growth in protoplanetary disks should
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Efficient Cosmic Ray Ion Production in Young Supernova Remnants
The strong shocks in young supernova remnants (SNRs) should accelerate cosmic rays (CRs) and no doubt exists that relativistic electrons
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Electromagnetic Radiation From The Accelerating Universe
The acceleration of the expansion of the universe has been argued for by several research groups. If the universe is
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Electroweak-Scale Excess Cross-Sections in the Sextet Quark ``Standard Model''
When the Higgs sector of the standard model is replaced by a flavor doublet of color sextet quarks, dynamical electroweak
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Formation of massive stars and black holes in self-gravitating AGN discs, and gravitational waves in LISA band
We propose a scenario in which massive stars form at the outer edges of an AGN accretion disc. We analyze
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Formation of Massive Stars via Accretion
The collapse of massive molecular clumps can produce high mass stars, but the evolution is not simply a scaled-up version
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Global Electrophonic Fireball Survey: a review of witness reports - I
Despite more than 300 years since its first scientific description, the phenomenon of electrophonic sounds from meteors are still eluding
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High Energy Cosmic Rays, Gamma Rays And Neutrinos From Jetted GRBs
Recent observations suggest that gamma ray bursts (GRBs) and their afterglows are produced in star formation regions in distant galaxies
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How do brown dwarves form?
We review and evaluate four mechanisms for forming brown dwarves: (i) dynamical ejection of a stellar embryo from its placental
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Insulator to Metal Transition Induced by Disorder in a Model for Manganites
The physics of manganites appears to be dominated by phase competition among ferromagnetic metallic and charge-ordered antiferromagnetic insulating states. Previous
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Jetted GRBs, Afterglows and SGRs from the Birth of Quark Stars
Recent studies suggest that when cold nuclear matter is compressed to high nuclear densities, diquarks with spin zero and antisymmetric
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