Search results for "SPECTRA"

showing 10 items of 3542 documents

The BeppoSAX 0.1–18 keV spectrum of the bright atoll source GX 9+1: an indication of the source distance

2005

We report the results of a long, 350 ks, BeppoSAX observation of the bright atoll source GX 9+1 in the 0.12-18 keV energy range. During this observation GX 9+1 showed a large count rate variability in its lightcurve. From its color-color diagram we selected six zones and extracted the source energy spectrum from each zone. We find that the model, composed of a blackbody plus a Comptonized component absorbed by an equivalent hydrogen column of ~1.4 ¿ 1022 cm-2, fits the spectra in the energy range 1-18 keV well; however, below 1 keV a soft excess is present. We find that the spectrum of GX 9+1, in the 0.12-18 keV energy range, is well fitted by the model above, if we use an equivalent hydrog…

PhysicsX-ray binaryAstronomyAstronomy and AstrophysicsAstrophysicsLight curveSpectral lineLuminosityInterstellar mediumNeutron starStarssymbols.namesakeSpace and Planetary ScienceEddington luminositysymbolsAstronomy & Astrophysics
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High-Energy pulse profile of the Transient X-ray Pulsar SAX J2103.5+4545

2005

In two recent INTEGRAL papers, Lutovinov et al. (2003) and Blay et al. (2004) report a timing and spectral analysis of the transient Be/X-ray pulsar SAX J2103.5+4545 at high energies (5--200 keV). In this work we present for the first time a study of the pulse profile at energies above 20 keV using INTEGRAL data. The spin-pulse profile shows a prominent (with a duty cycle of 14%) and broad (with a FWHM of ~ 51 s) peak and a secondary peak which becomes more evident above 20 keV. The pulsed fraction increases with energy from ~ 45% at 5--40 keV to ~ 80% at 40--80 keV. The morphology of the pulse profile also changes as a function of energy, consistent with variations in the spectral componen…

PhysicsX-rays : binariesScatteringAstrophysics::High Energy Astrophysical Phenomenapulsars : individual : SAX J2103.5+4545Astrophysics (astro-ph)Phase (waves)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsRadiationAstrophysicsSpectral linePulse (physics)Full width at half maximumPulsarbinaries : closeSpace and Planetary Scienceclose; pulsars : individual : SAX J2103.5+4545; X-rays : binaries [binaries]X-ray pulsar
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An X-shooter survey of star forming regions: Low-mass stars and sub-stellar objects

2011

We present preliminary results of our X-shooter survey in star forming regions. In this contribution we focus on sub-samples of young stellar and sub-stellar objects (YSOs) in the Lupus star forming region and in the TW Hya association. We show that the X-shooter spectra are suitable for conducting several parallel studies such as YSO + disk fundamental parameters, accretion and outflow activity in the very low-mass (VLM) and sub-stellar regimes, as well as magnetic activity in young VLM YSOs, and Li abundance determinations. The capabilities of X-shooter in terms of wide spectral coverage, resolution and limiting magnitudes, allow us to assess simultaneously the accretion/outflow, magnetic…

PhysicsYoung stellar objectBrown dwarfAstronomyAstronomy and AstrophysicsAstrophysicsAccretion (astrophysics)Spectral lineT Tauri starStarsaccretion accretion disks ISM: jets and outflows stars: formation stars: low-mass brown dwarfs stars: pre-main sequence T Tauri starsSpace and Planetary ScienceOutflowLow Massjets and outflows stars: formation stars: low-mass brown dwarfs stars: pre-main sequence T Tauri stars [accretion accretion disks ISM]
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Bose condensates at high angular momenta

2000

We exploit the analogy with the Quantum Hall (QH) system to study weakly interacting bosons in a harmonic trap. For a $\delta$-function interaction potential the ``yrast'' states with $L\ge N(N-1)$ are degenerate, and we show how this can be understood in terms of Haldane exclusion statistics. We present spectra for 4 and 8 particles obtained by numerical and algebraic methods, and demonstrate how a more general hard-core potential lifts the degeneracies on the yrast line. The exact wavefunctions for N=4 are compared with trial states constructed from composite fermions (CF), and the possibility of using CF-states to study the low L region at high N is discussed.

PhysicsYrastDegenerate energy levelsCondensed Matter (cond-mat)FOS: Physical sciencesCondensed MatterQuantum Hall effectAtomic and Molecular Physics and OpticsSpectral lineQuantum mechanicsComposite fermionAlgebraic numberWave functionBoson
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Atomic transitions of Rb, D2 line in strong magnetic fields: Hyperfine Paschen–Back regime

2014

An efficient $\lambda/2$-method ($\lambda$ is the resonant wavelength of laser radiation) based on nanometric-thickness cell filled with rubidium is implemented to study the splitting of hyperfine transitions of $^{85}$Rb and $^{87}$Rb $D_2$ lines in an external magnetic field in the range of $B =3$~kG -- 7~kG. It is experimentally demonstrated that at $B > 3$~kG from 38 (22) Zeeman transitions allowed at low $B$-field in $^{85}$Rb ($^{87}$Rb) spectra in the case of $\sigma^+$ polarized laser radiation there remain only 12 (8) which is caused by decoupling of the total electronic momentum $\textbf{J}$ and the nuclear spin momentum $\textbf{I}$ (hyperfine Paschen-Back regime). Note that at $…

PhysicsZeeman effectAtomic Physics (physics.atom-ph)FOS: Physical scienceschemistry.chemical_elementAtomic and Molecular Physics and OpticsSpectral linePhysics - Atomic Physics3. Good healthElectronic Optical and Magnetic MaterialsRubidiumMagnetic fieldMomentumsymbols.namesakeWavelengthchemistrysymbolsPhysics::Atomic PhysicsElectrical and Electronic EngineeringPhysical and Theoretical ChemistryAtomic physicsHyperfine structureLine (formation)Optics Communications
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Hyperfine Paschen-Back regime in alkali metal atoms: consistency of two theoretical considerations and experiment

2013

Simple and efficient "\lambda-method" and "\lambda/2-method" (\lambda is the resonant wavelength of laser radiation) based on nanometric-thickness cell filled with rubidium are implemented to study the splitting of hyperfine transitions of 85Rb and 87Rb D_1 line in an external magnetic field in the range of B = 0.5 - 0.7 T. It is experimentally demonstrated from 20 (12) Zeeman transitions allowed at low B-field in 85Rb (87Rb) spectra in the case of \sigma+ polarized laser radiation, only 6 (4) remain at B > 0.5 T, caused by decoupling of the total electronic momentum J and the nuclear spin momentum I (hyperfine Paschen-Back regime). The expressions derived in the frame of completely uncoupl…

PhysicsZeeman effectAtomic Physics (physics.atom-ph)chemistry.chemical_elementFOS: Physical sciencesStatistical and Nonlinear Physics01 natural sciencesAtomic and Molecular Physics and OpticsSpectral line3. Good healthRubidiumMagnetic fieldPhysics - Atomic Physics010309 opticsMomentumWavelengthsymbols.namesakechemistry0103 physical sciencessymbolsPhysics::Atomic PhysicsAtomic physics010306 general physicsHyperfine structureCircular polarization
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Broadening and intensity redistribution in theNa(3p)hyperfine excitation spectra due to optical pumping in the weak excitation limit

2008

Detailed analysis of spectral line broadening and variations in relative intensities of hyperfine spectral components due to optical pumping is presented. Hyperfine levels of sodium 3p1/2 and 3p3/2 levels are selectively excited in a supersonic beam at various laser intensities under the conditions when optical pumping time is shorter than transit time of atoms through the laser beam. The excitation spectra exhibit significant line broadening at laser intensities well below the saturation intensity, and redistribution of intensities of hyperfine spectral components is observed, which in some cases is contradicting with intuitive expectations. Theoretical analysis of the dynamics of optical …

PhysicsZeeman effectPhysics::OpticsLaserAtomic and Molecular Physics and OpticsSpectral linelaw.inventionOptical pumpingsymbols.namesakelawExcited statesymbolsPhysics::Atomic PhysicsAtomic physicsHyperfine structureExcitationRabi frequencyPhysical Review A
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Fluorescence of rubidium in a submicrometer vapor cell: spectral resolution of atomic transitions between Zeeman sublevels in a moderate magnetic fie…

2005

It is experimentally demonstrated that use of an extremely thin cell (ETC) with the thickness of a Rb atomic vapor column of ∼400 nm allows one to resolve a large number of individual transitions between Zeeman sublevels of the D1 line of 87Rb and 85Rb in the sub-Doppler fluorescence excitation spectra in an external magnetic field of ∼200 G. It is revealed that due to the peculiarities of the Zeeman effect for different hyperfine levels of Rb, all allowed transitions between magnetic sublevels can be clearly resolved for 87RbF_g = 1 --> F_e = 1, 2 and F_g = 2 --> F_e = 1, 2 fluorescence excitation. Also, relatively good spectral resolution can be achieved for 85RbF_g = 2 --> F_e = 2, 3 flu…

PhysicsZeeman effectchemistry.chemical_elementStatistical and Nonlinear PhysicsAtomic and Molecular Physics and OpticsRubidiumsymbols.namesakeNuclear magnetic resonancechemistryResonance fluorescenceExcited statesymbolsPhysics::Atomic PhysicsSpectral resolutionAtomic physicsLaser-induced fluorescenceHyperfine structureExcitationJournal of the Optical Society of America B
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STABILITY AND SPECTRA OF SMALL 3He-4He CLUSTERS

2005

Diffusion Monte Carlo calculations have been systematically performed to analyze the stability of small mixed 3 He -4 He clusters, as well as their excitation spectra. The picture that emerges is that of systems with strong shell effects whose binding and excitation energies are essentially determined by the monopole properties of an effective Hamiltonian.

Physics[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]Excitation spectraMagnetic monopolechemistry.chemical_elementStatistical and Nonlinear PhysicsCondensed Matter Physics01 natural sciencesSpectral line010305 fluids & plasmassymbols.namesakechemistry0103 physical sciencessymbolsDiffusion Monte CarloAtomic physics010306 general physicsHamiltonian (quantum mechanics)Mixed Helium clustersExcitationHeliumRecent Progress in Many-Body Theories
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The 1997 spectroscopic GEISA databank

1999

International audience; The current version GEISA-97 of the computer-accessible database system GEISA (Gestion et Etude des Informations Spectroscopiques Atmosphériques: Management and Study of Atmospheric Spectroscopic Information) is described. This catalogue contains 1,346,266 entries. These are spectroscopic parameters required to describe adequately the individual spectral lines belonging to 42 molecules (96 isotopic species) and located between 0 and 22,656 cm-1. The featured molecules are of interest in studies of the terrestrial as well as the other planetary atmospheres, especially those of the Giant Planets. GEISA-97 contains also a catalog of absorption cross-sections of molecule…

Physics[PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]Radiation010504 meteorology & atmospheric sciences0103 physical sciencesAstronomy010303 astronomy & astrophysics01 natural sciencesSpectroscopyAtomic and Molecular Physics and OpticsSpectral line0105 earth and related environmental sciencesWeb site
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