Search results for "X-rays."

showing 10 items of 443 documents

Long-term X-ray variability of the microquasar system LS 5039/RX J1826.2−1450

2003

We report on the results of the spectral and timing analysis of a BeppoSAX observation of the microquasar system LS 5039/RX J1826.2-1450. The source was found in a low-flux state with Fx(1-10 keV)= 4.7 x 10^{-12} erg cm^{-2} s^{-1}, which represents almost one order of magnitude lower than a previous RXTE observation 2.5 years before. The 0.1--10 keV spectrum is described by an absorbed power-law continuum with photon-number spectral index Gamma=1.8+-0.2 and hydrogen column density of NH=1.0^{+0.4}_{-0.3} x 10^{22} cm^{-2}. According to the orbital parameters of the system the BeppoSAX observation covers the time of an X-ray eclipse should one occur. However, the 1.6-10 keV light curve does…

HydrogenVariable starschemistry.chemical_elementFOS: Physical sciencesAstrophysicsCompact starAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICAAccretion rateRadio astronomyQuasarsQuàsarsEstels binaris de raigs XOrbital elementsPhysicsSpectral indexRX J1826.2−1450Astrophysics (astro-ph)X-rayIndividual Star ; LS 5039 ; RX J1826.2−1450 ; 3EG J1824−1514 – X-rays ; Variable stars ;; General–radio continuumAstronomy and AstrophysicsIndividual StarLight curveGeneral–radio continuum:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]StarsEstelsX-ray binarieschemistrySpace and Planetary ScienceRadioastronomiaLS 50393EG J1824−1514 – X-raysUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniaOrder of magnitude:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
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X-ray Emission Mechanisms in Herbig - Haro objects .

2006

ISM: Herbig-Haro objects ISM: individual objects: HH 154 ISM: jets and outflows X-rays: ISM
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Shock-cloud interactions in the Vela SNR: preliminary results of an XMM-Newton observation

2004

ISM: individual objectISM: structureVela supernova remnantISM: cloudsX-rays: ISMISM: supernova remnant
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Modeling the mixed-morphology supernova remnant IC 443. Origin of its complex morphology and X-ray emission

2020

The morphology and the distribution of material observed in SNRs reflect the interaction of the SN blast wave with the ambient environment, the physical processes associated with the SN explosion and the internal structure of the progenitor star. IC 443 is a MM SNR located in a quite complex environment: it interacts with a molecular cloud in the NW and SE areas and with an atomic cloud in the NE. In this work we aim at investigating the origin of the complex morphology and multi-thermal X-ray emission observed in SNR IC 443, through the study of the effect of the inhomogeneous ambient medium in shaping its observed structure, and the exploration of the main parameters characterizing the re…

ISM: individual objects: IC 443Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesContext (language use)Astrophysics01 natural sciencesPulsar wind nebulaSpectral lineSettore FIS/05 - Astronomia E Astrofisica0103 physical sciencesEjectaSupernova remnant010303 astronomy & astrophysicsBlast waveAstrophysics::Galaxy AstrophysicsISM: supernova remnantsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsMolecular cloudAstronomy and AstrophysicsX-rays: ISMSupernovaSpace and Planetary ScienceHydrodynamicsPulsars: individual: CXOU J061705.3+222127Astrophysics - High Energy Astrophysical Phenomena
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Investigation of pH-Responsiveness inside Lipid Nanoparticles for Parenteral mRNA Application Using Small-Angle X-ray Scattering.

2020

Messenger ribonucleic acid (mRNA)-based nanomedicines have shown to be a promising new lead in a broad field of potential applications such as tumor immunotherapy. Of these nanomedicines, lipid-based mRNA nanoparticles comprising ionizable lipids are gaining increasing attention as versatile technologies for fine-tuning toward a given application, with proven potential for successful development up to clinical practice. Still, several hurdles have to be overcome to obtain a drug product that shows adequate mRNA delivery and clinical efficacy. In this study, pH-induced changes in internal molecular organization and overall physicochemical characteristics of lipoplexes comprising ionizable li…

In situPhospholipidNanoparticle02 engineering and technology010402 general chemistry01 natural sciencesDegree of ionizationchemistry.chemical_compoundElectrochemistryGeneral Materials ScienceRNA MessengerParticle SizeSpectroscopyChemistrySmall-angle X-ray scatteringX-RaysRNASurfaces and InterfacesHydrogen-Ion Concentration021001 nanoscience & nanotechnologyCondensed Matter PhysicsFluorescence0104 chemical sciencesMembraneBiophysicsNanoparticles0210 nano-technologyLangmuir : the ACS journal of surfaces and colloids
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Unveiling the nature of six HMXBs through IR spectroscopy

2008

The International Gamma-Ray Astrophyiscs Laboratory (INTEGRAL) is discovering a large number of new hard X-ray sources, many of them being HMXBs. The identification and spectral characterization of their optical/infrared counterparts is a necessary step to undertake detailed study of these systems. In particular, the determination of the spectral type is crucial in the case of the new class of Supergiant Fast X-ray Transients (SFXTs), which show X-ray properties common to other objects. We used the ESO/NTT SofI spectrograph to observe proposed IR counterparts to HMXBs, obtaining Ks medium resolution spectra (R = 1320) with a S/N >= 100. We classified them through comparison with publishe…

InfraredAstrophysics::High Energy Astrophysical PhenomenaExtinction (astronomy)FOS: Physical sciencesInfrared spectroscopyAstrophysicsAstrophysicsStellar classificationSpectral line:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Fuentes de Rayos X [UNESCO]UNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Fuentes de Rayos XSpectroscopySpectrographAstrophysics::Galaxy AstrophysicsPhysicsAstrophysics (astro-ph)Astronomy and AstrophysicsAccretion accretion disksX-rays : binaries; Stars : supergiants; Accretion accretion disks; Infrared : starsSpace and Planetary Sciencestars [Infrared]binaries [X-rays]UNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::EstrellasSupergiantsupergiants [Stars]:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Estrellas [UNESCO]Astronomy & Astrophysics
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The Be/X-ray binary LS 992/RX J0812.4-3114: Physical parameters and long-term variability

2000

We present the first long-term optical and infrared study of the optical counterpart to the source RX J0812.4-3114, an X-ray pulsar with a Be type companion. During the period covered by the observations the profile of some Balmer lines changed from absorption to emission and back again to absorption. Contemporaneously, the infrared magnitudes varied by more than 0.8 mag. This long-term variability is interpreted as the formation and subsequent dissipation of the Be star's disc. The building up of the disc ended up in an active X-ray state characterised by regular outbursts occurring at 80 day intervals. The overall duration of the formation/dissipation of the disc is found to be < 4.3 year…

InfraredBe starAstrophysics::High Energy Astrophysical PhenomenaX-ray binaryFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICALS 992/RX J0812.4-3114Astrophysicssymbols.namesakePulsarX-raysAstrophysics::Solar and Stellar AstrophysicsAbsorption (electromagnetic radiation)Astrophysics::Galaxy AstrophysicsPhysicsAstrophysics (astro-ph)BinariesIndividual star ; LS 992/RX J0812.4-3114 ; Binaries ; Pulsars Emission-line ; Be ; X-raysBalmer seriesAstronomy and AstrophysicsBeCircumstellar envelopeDissipation:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]Space and Planetary SciencesymbolsIndividual starPulsars Emission-lineAstrophysics::Earth and Planetary AstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
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The structural versatility of proton sponge bismuth halides

2022

Hybrid halometalates containing lead, tin, bismuth and antimony and organic cations have recently shown a bevy of interesting photophysical properties. Aiming at finding chemically stable and thermally inert species, three halobismutate species of this class, crystallized with proton sponge-derived cations (PRSH), have been isolated as microcrystalline powders by mixing 1,8-bis(dimethylamino)-naphthalene (proton sponge, or PRS) and bismuth oxide in concentrated HX acids (X ​= ​Cl, Br and I). The two isomorphous (PRSH)3Bi2X9 (X ​= ​Br, I) species, containing isolated [Bi2X9]3- anions, are triclinic at room temperature and convert upon heating into a monoclinic structure through a displacive …

Inorganic ChemistryBismuth halidesPowder diffractionSettore CHIM/03 - Chimica Generale E InorganicaCrystal structureProton spongeSynchrotron X-raysMaterials ChemistryCeramics and CompositesPhysical and Theoretical ChemistryCondensed Matter PhysicsElectronic Optical and Magnetic Materials
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Intra- vs Intermolecular Aurophilic Contacts in Dinuclear Gold(I) Compounds: Impact on the Population of the Triplet Excited State.

2022

Two series of dinuclear gold(I) complexes that contain two Au–chromophore units (chromophore = dibenzofurane or dimethylfluorene) connected through a diphosphane bridge that differs in the flexibility and length (diphosphane = dppb for 1,4-bis(diphenylphosphino)butane, DPEphos for bis[(2-diphenylphosphino)phenyl]ether, xanthphos for 4,5-bis(diphenylphosphino)-9,9-dimethylxanthene, and BiPheP for 2,2′-bis(diphenylphosphino)-1,1′-biphenyl) have been synthesized and structurally characterized. Their photophysical properties have been carefully investigated, paying attention to the role of the presence, or absence, of aurophilic contacts and their nature (intra- or intermolecular character). Th…

Inorganic Chemistryabsorptiocrystal structurereaction productsX-raysröntgensäteilymolekyylitPhysical and Theoretical Chemistrykidetiedeabsorptionmolecular interactionsInorganic chemistry
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Carbon ions and X‑rays induce pro‑inflammatory effects in 3D oral mucosa models with and without PBMCs.

2014

Oral mucositis is a severe complication of radiotherapy. Hence, it may constitute a serious medical safety risk for astronauts during extended space flights, such as missions to Mars, during which they are exposed to heavy-ion irradiation. For risk assessment of developing radiation-induced mucositis, a three-dimensional (3D) organotypic oral mucosa model was irradiated with 12C heavy ions or X‑rays. The present study focused mainly on early radiation‑induced effects, such as the activation of nuclear factor κB (NFκB) and the expression or release of pro-inflammatory marker molecules. The 3D oral mucosa models with or without peripheral blood mononuclear cells (PBMCs) were irradiated with X…

KeratinocytesCancer ResearchDNA damageBiologyPeripheral blood mononuclear cellModels BiologicalmedicineMucositisHumansHeavy IonsInterleukin 8Oral mucosaCells CulturedX-RaysMouth MucosaInterleukinGeneral Medicinemedicine.diseaseCarbonCoculture TechniquesOrganoidsmedicine.anatomical_structureOncologyApoptosisToxicityCancer researchLeukocytes MononuclearCytokinesDNA DamageOncology reports
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