Search results for "emission"

showing 10 items of 2441 documents

Accretion in strong field gravity with eXTP

2019

In this paper we describe the potential of the enhanced X-ray Timing and Polarimetry (eXTP) mission for studies related to accretion flows in the strong field gravity regime around both stellar-mass and supermassive black-holes. eXTP has the unique capability of using advanced 'spectral-timing-polarimetry' techniques to analyze the rapid variations with three orthogonal diagnostics of the flow and its geometry, yielding unprecedented insight into the inner accreting regions, the effects of strong field gravity on the material within them and the powerful outflows which are driven by the accretion process.

ACTIVE GALACTIC NUCLEIAccretionaccretion; black holes physics; X-ray; Physics and Astronomy (all)black holes physicAstronomyAstrophysics::High Energy Astrophysical PhenomenaBlack holes physicsPolarimetryFOS: Physical sciencesBLACK-HOLE SPINGeneral Physics and AstronomyStrong fieldAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesX-rayPhysics and Astronomy (all)ELECTROMAGNETIC EMISSIONSettore FIS/05 - Astronomia e Astrofisicablack holes physicsaccretion0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010306 general physics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)XMM-NEWTONPhysicsLENS-THIRRING PRECESSION[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]QUASI-PERIODIC OSCILLATIONS[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]IRON KAccretion (astrophysics)X ray[SDU]Sciences of the Universe [physics]ULTRA-FAST OUTFLOWSAstrophysics::Earth and Planetary AstrophysicsSPECTRAL FEATURESAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]X-RAY BINARIESScience China Physics, Mechanics & Astronomy
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Thermal induced conformational changes involved in the aggregation of beta-lactoglobulin

2005

Aggregation of proteins appears to be associated most often with conformational and structural changes that lead to exposure of some apolar residues. Depending on the native structure of the protein in exam, aggregation is a process that involves different mechanisms, whose time of occurrence and interplay can depend upon temperature. To single out information about the multistages of the aggregation pathway, here we investigate the thermally induced conformational and structural changes of the beta-lactoglobulin (BLG). The experimental approach consists in studying steady-state fluorescence spectra of intrinsic chromophores, two tryptophans, and Anylino-Naphthalene-Sulfonate dye (ANS) mole…

ANS emissionBeta-lactoglobulinProtein aggregationRayleigh scatteringCircular dichroismConformational changeFluorescence
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Binding mode analysis of ABCA7 for the prediction of novel Alzheimer's disease therapeutics

2021

Graphical abstract

ATP Adenosine-triphosphateNBD nucleotide binding domainGSH reduced glutathionePolypharmacologyAlzheimer’s disease (AD)ATP-binding cassette transporterHTS high-throughput screeningBiochemistryABCA7Structural BiologyPLIF protein ligand interactionMSD membrane spanning domainPDB protein data bankTM transmembrane helixABC ATP-binding cassetteMultitarget modulation (PANABC)RMSD root mean square distanceABC transporter (ABCA1 ABCA4 ABCA7)Computer Science ApplicationsMOE Molecular Operating EnvironmentPharmacophoreSNP single-nucleotide polymorphismBiotechnologyResearch ArticleBBB blood-brain barrierBiophysicsDrug designComputational biologyBiologyAD Alzheimer’s diseasePET positron emission tomographyIC intracellular helixAPP amyloid precursor proteincryo-EM cryogenic-electron microscopyGeneticsHomology modelingBinding siteRational drug design and developmentComputingMethodologies_COMPUTERGRAPHICSNBD-cholesterol 7-nitro-2-13-benzoxadiazol-4-yl-cholesterolTransporterPSO particle swarm optimizationPET tracer (PETABC)ECD extracellular domainR-domain/region regulatory domain/regionABCA1biology.proteinEH extracellular helixTP248.13-248.65BODIPY-cholesterol 44-difluoro-4-bora-3a4a-diaza-s-indacene-cholesterolComputational and Structural Biotechnology Journal
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Regioselective Hydrogenation of a 60-Carbon Nanographene Molecule toward a Circumbiphenyl Core.

2019

Regioselective peripheral hydrogenation of a nanographene molecule with 60 contiguous sp2 carbons provides unprecedented access to peralkylated circumbiphenyl (1). Conversion to the circumbiphenyl core structure was unambiguously validated by MALDI-TOF mass spectrometry, NMR, FT-IR, and Raman spectroscopy. UV–vis absorption spectra and DFT calculations demonstrated the significant change of the optoelectronic properties upon peripheral hydrogenation. Stimulated emission from 1, observed via ultrafast transient absorption measurements, indicates potential as an optical gain material.

Absorption spectroscopyChemistryCommunicationChemistry (all)RegioselectivityGeneral Chemistry010402 general chemistryMass spectrometryPhotochemistryCatalysis; Chemistry (all); Biochemistry; Colloid and Surface Chemistry01 natural sciencesBiochemistryCatalysis0104 chemical sciencesCatalysissymbols.namesakeColloid and Surface ChemistryUltrafast laser spectroscopysymbolsMoleculeStimulated emissionRaman spectroscopyJournal of the American Chemical Society
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Investigation of molecular dimers by ensemble and single molecule spectroscopy

2002

International audience; We have investigated molecular dimers with different electronic coupling strengths by bulk and single molecule spectroscopy. In one of the dimers the two monomers (perylene-monoimide) are directly connected via a single bond while in the other one they are separated by the benzil motif. The close proximity of the monomers in the first case gives rise to excitonic band splitting which is clearly observable in the bulk absorption spectra. For the benzil structure the electronic interactions are governed by Förster-type energy hopping between the monomers. Fluorescence intensity trajectories at the single molecule level show one-step and two-step bleaching behaviour whi…

Absorption spectroscopyExcitonBiophysics010402 general chemistryPhotochemistry01 natural sciencesBiochemistrychemistry.chemical_compoundElectronic interactionsSingle bondMolecule[CHIM]Chemical SciencesEmission spectrum010405 organic chemistryGeneral ChemistryCondensed Matter PhysicsMolecular aggregatesAtomic and Molecular Physics and Optics0104 chemical sciences3. Good healthCoupling (physics)MonomerchemistryChemical physicsExcitonsBenzilSingle molecule spectroscopy
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On the Low-Lying Excited States ofsym-Triazine-Based Herbicides

2005

We report a joint computational and luminescence study on the low-lying excited states of sym-triazines, namely, 1,3,5-triazine (1) and the ubiquitous herbicides atrazine [6-chloro-N2-ethyl-N4-isopropyl-1,3,5-triazine-2,4-diamine (2)] and ametryn [6-methylthio-N2-ethyl-N4-isopropyl-1,3,5-triazine-2,4-diamine (3)]. Geometrical structures, energetics, and transition and state properties of I and 2 were computed at the TD-DFT, CASSCF, and CASPT2 levels of theory. The fluorescence and phosphorescence emission spectra, lifetimes, and fluorescence quantum yields were measured for the three compounds, and from these, the energies of the lowest excited states and their corresponding radiative rates…

Absorption spectroscopyQuantum yieldPhotochemistryMolecular physicsAbsorptionAb initio quantum chemistry methodsOscillometryPressureRadiative transferEmission spectrumPhysical and Theoretical ChemistryMolecular StructureChemistry PhysicalHerbicidesTriazinesChemistryTemperatureHydrogen-Ion ConcentrationModels TheoreticalAtomic and Molecular Physics and OpticsSpectrometry FluorescenceModels ChemicalSpectrophotometryExcited stateAtrazineIndicators and ReagentsPhosphorescenceLuminescenceSoftwareChemPhysChem
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Transition-Edge Sensors for Particle Induced X-ray Emission Measurements

2013

In this paper we present a new measurement setup, where a transitionedge sensor detector array is used to detect X-rays in particle induced X-ray emission measurements with a 2 MeV proton beam. Transition-edge sensors offer orders of magnitude improvement in energy resolution compared to conventional silicon or germanium detectors, making it possible to recognize spectral lines in materials analysis that have previously been impossible to resolve, and to get chemical information from the elements. Our sensors are cooled to the operation temperature (65 mK) with a cryogen-free adiabatic demagnetization refrigerator, which houses a specially designed X-ray snout that has a vacuum tight window…

Accelerator Physics (physics.acc-ph)Physics - Instrumentation and DetectorsMaterials scienceProtonPhysics::Instrumentation and DetectorsOrders of magnitude (temperature)FOS: Physical scienceschemistry.chemical_elementGermaniumRadiationSpectral lineOpticsGeneral Materials Scienceparticle induced X-ray emission (PIXE)Emission spectrumbusiness.industryDetectorInstrumentation and Detectors (physics.ins-det)transition-edge sensorCondensed Matter PhysicsAtomic and Molecular Physics and OpticsFull width at half maximumchemistryPhysics - Accelerator PhysicsbusinessTESJournal of Low Temperature Physics
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Spectral and timing properties of IGR J00291+5934 during its 2015 outburst

2016

We report on the spectral and timing properties of the accreting millisecond X-ray pulsar IGR J00291+5934 observed by XMM-Newton and NuSTAR during its 2015 outburst. The source is in a hard state dominated at high energies by a comptonization of soft photons ($\sim0.9$ keV) by an electron population with kT$_e\sim30$ keV, and at lower energies by a blackbody component with kT$\sim0.5$ keV. A moderately broad, neutral Fe emission line and four narrow absorption lines are also found. By investigating the pulse phase evolution, we derived the best-fitting orbital solution for the 2015 outburst. Comparing the updated ephemeris with those of the previous outbursts, we set a $3��$ confidence leve…

AccretionAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics01 natural sciencesPulsar0103 physical sciencesneutron; X-rays: binaries; Astronomy and Astrophysics; Space and Planetary Science [Accretion; Accretion discs; Stars]Emission spectrumSpectroscopy010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsAccretion (meteorology)010308 nuclear & particles physicsAstronomy and AstrophysicsAstronomy and AstrophysicOrbital periodX-rays: binarieStars: neutronNeutron starAmplitude13. Climate actionSpace and Planetary ScienceAccretion discAstrophysics - High Energy Astrophysical PhenomenaEnergy (signal processing)Monthly Notices of the Royal Astronomical Society
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INTEGRAL observations of the peculiar BeX System SAX J2103.5+4545

2004

We present an INTEGRAL data analysis of the X-ray transient \object{SAX J2103.5+4545} during two outbursts detected in December 2002. The INTEGRAL coordinates and error circle agree with the position of the recently proposed optical counterpart. A power-law plus cut-off model provided a good fit to the 4-150 keV spectrum yielding a photon index of 1.0+-0.1, a cut-off energy E_cut=7.6+-2.0 keV and a folding energy E_fold=30.9+-2.5 keV. The X-ray luminosity in the 4-150 keV energy range was found to be 6.0x10^36 erg/s, assuming a distance of 6.5 kpc. This luminosity, together with the derived photon index, indicate that the source is in a bright state. A 354.9$+-0.5 second pulse period is mea…

AccretionPhotonAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesValue (computer science)AstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICAAstrophysicsLuminosityPulse periodPosition (vector)X-raysBright statePhysicsRange (particle radiation)Astrophysics (astro-ph)BinariesSAX J2103.5+4545 [Pulsars]BeAstronomy and Astrophysics:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]Space and Planetary ScienceAccretion disksUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniaEmission-lineAccretion ; Accretion disks ; Binaries ; Emission-line ; Be ; Pulsars : SAX J2103.5+4545 ; X-rays ; Binaries:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]Energy (signal processing)Astronomy & Astrophysics
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Redshifted X-rays from the material accreting onto TW Hya: evidence of a low-latitude accretion spot

2017

High resolution spectroscopy, providing constraints on plasma motions and temperatures, is a powerful means to investigate the structure of accretion streams in CTTS. In particular, the accretion shock region, where the accreting material is heated to temperatures of a few MK as it continues its inward bulk motion, can be probed by X-ray spectroscopy. To attempt to detect for the first time the motion of this X-ray-emitting post-shock material, we searched for a Doppler shift in the deep Chandra/HETGS observation of the CTTS TW Hya. This test should unveil the nature of this X-ray emitting plasma component in CTTS, and constrain the accretion stream geometry. We searched for a Doppler shift…

AccretionTechniques: spectroscopicFOS: Physical sciencesAstrophysics01 natural sciencesSettore FIS/05 - Astronomia E Astrofisica0103 physical sciencesTW HydraeX-rays: starEmission spectrumSpectroscopy010303 astronomy & astrophysicsStars: variables: T TauriSolar and Stellar Astrophysics (astro-ph.SR)PhysicsPhotosphereLine-of-sight010308 nuclear & particles physicsHerbig Ae/BeAstronomy and AstrophysicsAstronomy and AstrophysicRedshiftAccretion (astrophysics)T Tauri starAstrophysics - Solar and Stellar AstrophysicsAccretion diskSpace and Planetary ScienceStars: pre-main sequence
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