Search results for "ARTICLES"

showing 10 items of 9626 documents

Non-thermal radiation from a pulsar wind interacting with an inhomogeneous stellar wind

2017

Binaries hosting a massive star and a non-accreting pulsar are powerful non-thermal emitters due to the interaction of the pulsar and the stellar wind. The winds of massive stars are thought to be inhomogeneous, which could have an impact on the non-thermal emission. We study numerically the impact of the presence of inhomogeneities or clumps in the stellar wind on the high-energy non-thermal radiation of high-mass binaries hosting a non-accreting pulsar. We compute the trajectories and physical properties of the streamlines in the shocked pulsar wind without clumps, with a small clump, and with a large one. This information is used to compute the synchrotron and inverse Compton emission fr…

Be starAstrophysics::High Energy Astrophysical PhenomenaPopulationEstels binarisFOS: Physical sciencesSynchrotron radiationAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics7. Clean energy01 natural sciencesRaigs gammaDouble starsPulsar0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsAdiabatic processeducation010303 astronomy & astrophysicsPulsarsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicseducation.field_of_studyHidrodinàmica010308 nuclear & particles physicsGamma raysAstronomy and AstrophysicsPúlsarsParticle accelerationStarsAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary ScienceThermal radiationHydrodynamicsAstrophysics - High Energy Astrophysical PhenomenaAstronomy & Astrophysics
researchProduct

Activity from the Be/X-ray binary system V0332+53 during its intermediate-luminosity outburst in 2008

2015

Aims: We present a study of the Be/X-ray binary system V 0332+53 with the main goal of characterizing its behavior mainly during the intermediate-luminosity X-ray event on 2008. In addition, we aim to contribute to the understanding of the global behavior of the donor companion by including optical data from our dedicated campaign starting on 2006. Methods: V 0332+53 was observed by RXTE and Swift during the decay of the intermediate-luminosity X-ray outburst of 2008, as well as with Suzaku before the rising of the third normal outburst of the 2010 series. In addition, we present recent data from the Spanish ground-based astronomical observatories of El Teide (Tenerife), Roque de los Muchac…

Be starAstrophysics::High Energy Astrophysical Phenomenageneral [Pulsars]X-ray binaryMagnetosphereFluxFOS: Physical sciencesAstrophysics01 natural sciencesLuminosityX-rays: binariesObservatoryindividual: V 0332+53 [Stars]0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsLine (formation)Stars: individual: V 0332+53PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsAstronomy and AstrophysicsPulsars: generalNeutron starSpace and Planetary Sciencebinaries [X-rays]Astrophysics - High Energy Astrophysical Phenomena
researchProduct

A study of the B and Be star population in the field of the LMC open cluster NGC 2004 with VLT-FLAMES

2005

Observations of hot stars belonging to the young cluster LMC-NGC2004 and its surrounding region have been obtained with the VLT-GIRAFFE facilities in MEDUSA mode. 25 Be stars were discovered; the proportion of Be stars compared to B-type stars is found to be of the same order in the LMC and in the Galaxy fields. 23 hot stars were discovered as spectroscopic binaries (SB1 and SB2), 5 of these are found to be eclipsing systems from the MACHO database, with periods of a few days. About 75% of the spectra in our sample are polluted by hydrogen (Halpha and Hgamma), [SII] and [NII] nebular lines. These lines are typical of HII regions. They could be associated with patchy nebulosities with a bi-m…

Be starPopulationFOS: Physical sciencesAstrophysicsAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICA01 natural sciencesbinaries: eclipsing [Stars]Spectral lineStars: early-type[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]ISM: nebular lines and bandsMagellanic Clouds [Galaxies]early-type [Stars]Stars: binaries: spectroscopic0103 physical sciencesCluster (physics)education010303 astronomy & astrophysicsStars: binaries: eclipsingPhysicseducation.field_of_study[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsStars: emission-lineAstrophysics (astro-ph)Stars: early-type ; Stars: emission-line Be ; Galaxies: Magellanic Clouds ; Stars: binaries: spectroscopic ; Stars: binaries: eclipsing ; ISM: lines and bandsAstronomy and AstrophysicsBeGalaxies: Magellanic CloudsGalaxyRadial velocityStarsbinaries: spectroscopic [Stars]Space and Planetary Scienceemission-line Be [Stars][SDU]Sciences of the Universe [physics]lines and bands [ISM]:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]Open cluster
researchProduct

Bibliographie nodiériste en ligne : œuvres et paratextes critiques

2011

Bibliographie en ligne autour des œuvres de Charles Nodier progressivement mise en place sur le site des Cahiers d'études nodiéristes. Projet d'envergure évolutif et chronologiquement rétrospectif : sa première étape couvrant la période 2000 à nos jours est opérationnelle.URL : http://www.cahiers-nodieristes.fr/bibliographie.html

Bibliographie informatiséeBibliographie en ligneThèses sur Charles NodierNodier studies -- ThesisHistoire de la critique littéraireRomantisme littérature[SHS.LITT] Humanities and Social Sciences/LiteratureNodier studies -- MasterNodier studies -- PhDMétabibliographieLittérature romantiqueCritique littéraireNodier reviewLittérature française -- 19e siècle -- Thèmes motifs -- actes de congrèsLittérature française -- 19e siècle -- Histoire et critiqueÉtudes sur Charles NodierEssais sur Charles NodierMarie Nodier 1811-1893Articles sur Charles NodierLinguistique des originesAcadémie française[SHS.LANGUE] Humanities and Social Sciences/LinguisticsÉtudes nodiéristesŒuvres de Marie Mennessier-NodierCharles Nodier 1780-1844Littérature française -- 19e siècle -- ThèmesŒuvres de Charles NodierLittérature française -- 19e siècle -- Thèmes motifs -- journées d'étude
researchProduct

Membrane fatty acid composition and fluidity are involved in the resistance to freezing of Lactobacillus buchneri R1102 and Bifidobacterium longum R0…

2015

International audience; Determinations of membrane fatty acid composition and fluidity were used together with acidification activity and viability measurements to characterize the physiological state after freezing of Lactobacillus buchneri R1102 and Bifidobacterium longum R0175 cells harvested in the exponential and stationary growth phases. For both strains, lower membrane fluidity was achieved in cells harvested in the stationary growth phase. This change was linked to a lower unsaturated-to-saturated fatty acid ratio for both strains and a higher cyclic-to-saturated fatty acid ratio for L. buchneri R1102 alone. These membrane properties were linked to survival and to maintenance of aci…

Bifidobacterium longum[SDV.BIO]Life Sciences [q-bio]/BiotechnologyMembrane FluidityBioengineeringApplied Microbiology and BiotechnologyBiochemistryCell membraneLactobacillusFreezing[SDV.IDA]Life Sciences [q-bio]/Food engineeringmedicineMembrane fluidityResearch ArticlesBifidobacteriumLactobacillus buchnerichemistry.chemical_classificationMicrobial ViabilitybiologyCell MembraneFatty Acids[ SDV.IDA ] Life Sciences [q-bio]/Food engineeringFatty acid[ SDV.BIO ] Life Sciences [q-bio]/Biotechnologybiology.organism_classificationLactobacillusmedicine.anatomical_structurechemistryBiochemistrySaturated fatty acidBifidobacteriumBiotechnology
researchProduct

Cosmic Dark Radiation and Neutrinos

2013

New measurements of the cosmic microwave background (CMB) by the Planck mission have greatly increased our knowledge about the universe. Dark radiation, a weakly interacting component of radiation, is one of the important ingredients in our cosmological model which is testable by Planck and other observational probes. At the moment, the possible existence of dark radiation is an unsolved question. For instance, the discrepancy between the value of the Hubble constant, H-0, inferred from the Planck data and local measurements of H-0 can to some extent be alleviated by enlarging the minimal ACDM model to include additional relativistic degrees of freedom. From a fundamental physics point of v…

Big BangNuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Article SubjectAge of the universeDark matterFOS: Physical sciencesLambda-CDM modelAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesBayron acoustic-Oscillationssymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)Analytic approach0103 physical sciencesPlanck010306 general physicsPhysicsAstrophysics - Cosmology and Extragalactic Astrophysics010308 nuclear & particles physicsHot dark matterFísicalcsh:QC1-999High Energy Physics - Phenomenology13. Climate actionDark radiationDark energysymbolslcsh:PhysicsAstrophysics - Cosmology and Nongalactic AstrophysicsAdvances in High Energy Physics
researchProduct

Uncertainty on w from large-scale structure

2012

We find that if we live at the center of an inhomogeneity with total density contrast of roughly 0.1, dark energy is not a cosmological constant at 95% confidence level. Observational constraints on the equation of state of dark energy, w, depend strongly on the local matter density around the observer. We model the local inhomogeneity with an exact spherically symmetric solution which features a pressureless matter component and a dark-energy fluid with constant equation of state and negligible sound speed, that reaches a homogeneous solution at finite radius. We fit this model to observations of the local expansion rate, distant supernovae and the cosmic microwave background. We conclude …

Big BangPhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)ta114010308 nuclear & particles physicsEquation of state (cosmology)Scalar field dark matterFOS: Physical sciencesAstronomy and AstrophysicsLambda-CDM modelGeneral Relativity and Quantum Cosmology (gr-qc)Cosmological constantAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesGeneral Relativity and Quantum CosmologyComputational physicsThermodynamics of the universeSpace and Planetary ScienceQuantum mechanics0103 physical sciencesDark energy010303 astronomy & astrophysicsDark fluidAstrophysics - Cosmology and Nongalactic Astrophysics
researchProduct

De novo design of protein kinase inhibitors by in silico identification of hinge region-binding fragments.

2013

Protein kinases constitute an attractive family of enzyme targets with high relevance to cell and disease biology. Small molecule inhibitors are powerful tools to dissect and elucidate the function of kinases in chemical biology research and to serve as potential starting points for drug discovery. However, the discovery and development of novel inhibitors remains challenging. Here, we describe a structure-based de novo design approach that generates novel, hinge-binding fragments that are synthetically feasible and can be elaborated to small molecule libraries. Starting from commercially available compounds, core fragments were extracted, filtered for pharmacophoric properties compatible w…

Binding SitesMolecular StructureProtein ConformationIntracellular Signaling Peptides and ProteinsArticlesProtein Serine-Threonine KinasesCrystallography X-RayMAP Kinase Kinase KinasesImmediate-Early ProteinsCSK Tyrosine-Protein KinaseMolecular Docking SimulationSmall Molecule Librariessrc-Family KinasesDrug DesignComputer SimulationProtein Kinase InhibitorsACS chemical biology
researchProduct

Aqueous phase/nanoparticles interface: hydroxypropyl cellulose adsorption and desorption triggered by temperature and inorganic salts

2012

The study highlighted the main forces driving the adsorption of hydroxypropyl cellulose (HPC) onto clay nanoparticles with a disk-like shape (Laponite RD). Modeling the isothermal titration calorimetry data provided the key thermodynamic properties, which enabled us to discuss the microscopic aspects contributing to the energetic and the entropic changes of the polymer adsorption at the nanoparticle/liquid interface. We evidenced that the process is strongly enthalpy-driven and that the interactions lead to constraints of the HPC configuration at interface. The functionalized nanoparticles enhanced the polymer solubility in water expanding the one-phase area of the binodal curve. Temperatur…

BinodalMaterials scienceHydroxypropyl cellulosenanoparticles interface cellulose calorimetryNanoparticleIsothermal titration calorimetryGeneral ChemistryPolymer adsorptionCondensed Matter Physicschemistry.chemical_compoundAdsorptionchemistryChemical engineeringDesorptionOrganic chemistrySolubilitySettore CHIM/02 - Chimica Fisica
researchProduct

Recent advances in smart biotechnology: Hydrogels and nanocarriers for tailored bioactive molecules depot

2017

Over the past ten years, the global biopharmaceutical market has remarkably grown, with ten over the top twenty worldwide high performance medical treatment sales being biologics. Thus, biotech R&D (research and development) sector is becoming a key leading branch, with expanding revenues. Biotechnology offers considerable advantages compared to traditional therapeutic approaches, such as reducing side effects, specific treatments, higher patient compliance and therefore more effective treatments leading to lower healthcare costs. Within this sector, smart nanotechnology and colloidal self-assembling systems represent pivotal tools able to modulate the delivery of therapeutics. A comprehens…

Bioactive molecules02 engineering and technologyHepatocellular-carcinoma cells01 natural sciencesMiceColloid and Surface ChemistryDrug Delivery SystemsCarbon nano materialNanotechnologyMolecular Targeted TherapyTransgenesRNA Small InterferingPatient complianceTransfer radical polymerizationMicro/nanocarrierMedical treatmentMicro/nanocarriersBioactive molecule deliveryHydrogelsSurfaces and Interfaces021001 nanoscience & nanotechnologyLiposomeBiopharmaceuticalOral deliverySelf-healing hydrogelsIntercellular Signaling Peptides and Proteins0210 nano-technologyAssembling peptide hydrogelsSurfaces and InterfaceNucleic-acid deliveryPlasmidsDiagnostic ImagingSolid lipid nanoparticlesNanotechnology010402 general chemistryAntibodiesSmall Molecule LibrariesCarbon nano-onionsIn-vivoAnimalsHumansPhysical and Theoretical Chemistrybusiness.industryDrug-delivery0104 chemical sciencesBiotechnologyHydrogelSettore CHIM/09 - Farmaceutico Tecnologico ApplicativoMolecular ProbesBioactive molecule delivery; Carbon nano materials; Hydrogels; Liposomes; Micro/nanocarriers; Surfaces and Interfaces; Physical and Theoretical Chemistry; Colloid and Surface ChemistryLiposomesNonviral gene deliveryCarbon nano materialsNanoparticlesBusinessNanocarriers
researchProduct