Search results for "Spectral"

showing 10 items of 3116 documents

Fundamental properties and atmospheric structure of the red supergiant VY CMa based on VLTI/AMBER spectro-interferometry

2012

We investigate the atmospheric structure and fundamental properties of the red supergiant VY CMa. We obtained near-infrared spectro-interferometric observations of VY CMa with spectral resolutions of 35 and 1500 using the AMBER instrument at the VLTI. The visibility data indicate the presence of molecular layers of water vapor and CO in the extended atmosphere with an asymmetric morphology. The uniform disk diameter in the water band around 2.0 mu is increased by \sim20% compared to the near-continuum bandpass at 2.20-2.25 mu and in the CO band at 2.3-2.5 mu it is increased by up to \sim50%. The closure phases indicate relatively small deviations from point symmetry close to the photospheri…

PhysicsFOS: Physical sciencesAstronomy and AstrophysicsAtmospheric modelAstrophysicsRadiusEffective temperatureAtmosphere of EarthAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceAngular diameterRed supergiantSpectral resolutionSolar and Stellar Astrophysics (astro-ph.SR)Water vapor
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Strong Chromatic Microlensing in HE0047-1756 and SDSS1155+6346

2014

We use spectra of the double lensed quasars HE0047-1756 and SDSS1155+6346 to study their unresolved structure through the impact of microlensing. There is no significant evidence of microlensing in the emission line profiles except for the Ly$\alpha$ line of SDSS1155+6346, which shows strong differences in the shapes for images A and B. However, the continuum of the B image spectrum in SDSS1155+6346 is strongly contaminated by the lens galaxy and these differences should be considered with caution. Using the flux ratios of the emission lines for image pairs as a baseline to remove macro-magnification and extinction, we have detected strong chromatic microlensing in the continuum measured by…

PhysicsFOS: Physical sciencesAstronomy and AstrophysicsQuasarAstrophysicsRest frameGravitational microlensingAstrophysics - Astrophysics of GalaxiesGalaxySpectral lineAmplitudeThin diskSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Emission spectrum
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Quons, coherent states and intertwining operators

2009

We propose a differential representation for the operators satisfying the q-mutation relation $BB^\dagger-q B^\dagger B=\1$ which generalizes a recent result by Eremin and Meldianov, and we discuss in detail this choice in the limit $q\to1$. Further, we build up non-linear and Gazeau-Klauder coherent states associated to the free quonic hamiltonian $h_1=B^\dagger B$. Finally we construct almost isospectrals quonic hamiltonians adopting the results on intertwining operators recently proposed by the author.

PhysicsFOS: Physical sciencesGeneral Physics and AstronomyMathematical Physics (math-ph)Intertwining operatorcoherent statesAlgebrasymbols.namesakeIsospectralQuonQuantum mechanicssymbolsCoherent statesHamiltonian (quantum mechanics)Settore MAT/07 - Fisica MatematicaMathematical Physics
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Extended SUSY quantum mechanics, intertwining operators and coherent states

2009

Abstract We propose an extension of supersymmetric quantum mechanics which produces a family of isospectral Hamiltonians. Our procedure slightly extends the idea of intertwining operators. Several examples of the construction are given. Further, we show how to build up vector coherent states of the Gazeau–Klauder type associated to our Hamiltonians.

PhysicsFOS: Physical sciencesGeneral Physics and AstronomyMathematical Physics (math-ph)SupersymmetryExtension (predicate logic)coherent statesType (model theory)supersimmetric quantum mechanicTheoretical physicsIsospectralMathematics::Mathematical PhysicsCoherent statesSupersymmetric quantum mechanicsSettore MAT/07 - Fisica MatematicaMathematical PhysicsPhysics Letters A
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Pulse Generation and Shaping Using Fiber Nonlinearities

2017

PhysicsFemtosecond pulse shapingOpticsFiber nonlinearitybusiness.industryFiberbusinessSpectral shapingPulse (physics)
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Iodine on a magnetized iron film evidence for a magnetic coupling

1993

Abstract Spin-resolved photoelectron spectra of iodine chemisorbed on a magnetized iron (110) surface have been taken using unpolarized VUV light. The partial spin spectra reveal the I 5p x and 5p z signals being split by up to 0.35 eV. This exchange splitting occurs due to hybridization of adsorbate and substrate bands as a consequence of the chemical bond of the halogen atoms to the iron surface.

PhysicsFerromagnetismX-ray photoelectron spectroscopyTransition metalChemical bondChemisorptionEnergy level splittingHalogenGeneral Physics and AstronomyAtomic physicsSpectral linePhysics Letters A
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Laser Resonance Chromatography of Superheavy Elements.

2020

Optical spectroscopy constitutes the historical path to accumulate basic knowledge on the atom and its structure. Former work based on fluorescence and resonance ionization spectroscopy enabled identifying optical spectral lines up to element 102, nobelium. The new challenges faced in this research field are the refractory nature of the heavier elements and the decreasing production yields. A new concept of ion-mobility-assisted laser spectroscopy is proposed to overcome the sensitivity limits of atomic structure investigations persisting in the region of the superheavy elements. The concept offers capabilities of both broadband-level searches and high-resolution hyperfine spectroscopy of s…

PhysicsField (physics)Atomic Physics (physics.atom-ph)General Physics and Astronomychemistry.chemical_elementFOS: Physical sciencesSuperheavy ElementsSynthetic element7. Clean energy01 natural sciencesSpectral line3. Good healthPhysics - Atomic Physicschemistry0103 physical sciencesddc:530NobeliumAtomic physics010306 general physicsSpectroscopyHyperfine structureRefractory (planetary science)Physical review letters
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Radiative Recombination in a Strong Laser Field

2006

Recent advances of radiative recombination in the presence of strong laser fields are reported. The intense laser radiation is found to introduce new relevant features, among which enhancement and control of the emitted X-ray spectra are the most important. The influence of the plasma medium in which the process generally takes place is considered as well. The results of the recent investigations shed new light on the laser assisted radiative recombination physics and give relevant indications concerning the possibilities to have effective slow electrons and to balance the plasma heating, as needed in important applications.

PhysicsField (physics)positroniumantihydrogen atomsElectronPlasmaRadiationLaserSpectral linelaw.inventionlawAntiprotonSpontaneous emissionAtomic physicsantiprotons
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The density of coronal plasma in active stellar coronae

2004

We have analyzed high-resolution X-ray spectra of a sample of 22 active stars observed with the High Energy Transmission Grating Spectrometer on {\em Chandra} in order to investigate their coronal plasma density. Densities where investigated using the lines of the He-like ions O VII, Mg XI, and Si XIII. While Si XIII lines in all stars of the sample are compatible with the low-density limit, Mg XI lines betray the presence of high plasma densities ($> 10^{12}$ cm$^{-3}$) for most of the sources with higher X-ray luminosity ($> 10^{30}$ erg/s); stars with higher $L_X$ and $L_X/L_{bol}$ tend to have higher densities at high temperatures. Ratios of O VII lines yield much lower densities …

PhysicsFilling factorAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)FluxOrder (ring theory)FOS: Physical sciencesAstronomy and AstrophysicsPlasmaAstrophysicsAstrophysicsSpectral lineLuminosityIonStarsSpace and Planetary ScienceAstrophysics::Solar and Stellar Astrophysicsplasmas stars: activity stars: coronae stars: late-type Sun: corona X-rays: stars
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X‐Ray Spectroscopy of the Unsteady Quiescent Corona of AD Leonis withChandra

2004

We present the analysis and interpretation of an observation of the flare star AD Leo (dM3e) with Chandra/LETG. The high resolution X-ray spectrum allowed us to infer the plasma emission measure distribution (EMD) vs. temperature, and the abundances of individual elements in the corona of this magnetically-active star, during a typical state characterized by significant variability but no large flaring event. We have also measured plasma densities at various temperatures using spectroscopic diagnostics provided by He-like triplets and Fe XXI lines. We show that the present EMD is similar to those previously obtained from EUVE spectra during quiescent and flaring states, confirming the long-…

PhysicsFilling factorAstrophysics::High Energy Astrophysical PhenomenaMetallicityAstrophysics (astro-ph)Flare starFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsPlasmaAstrophysicsCoronaSpectral lineStarsSpace and Planetary SciencePhysics::Space PhysicsAstrophysics::Solar and Stellar AstrophysicsIonization energyThe Astrophysical Journal
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