Search results for "X ray"

showing 10 items of 173 documents

The flaring afterglow of GRB 050730

2006

We present a detailed spectral and temporal analysis of Swift and XMM-Newton observations of GRB 050730. The X-ray afterglow of GRB 050730 was found to decline with time with intense flaring activity superimposed. Evidence of flaring activity in the early UVOT optical afterglow, simultaneous with that observed in the X-ray band, was found. Strong spectral evolution in the X-ray energy band during the flaring activity was present.

Afterglows X Rays XMM-Newton Telescope
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The F-type centres in YAG crystals

2001

The comparative study of optical properties of thermochemically reduced undoped YAG (Y3Al5O12) crystals is reported. A particular type of the centres often observed in YAG crystals synthesized as w...

Aluminium oxidesNuclear and High Energy PhysicsRadiationMaterials sciencePhotoluminescenceOpticsbusiness.industryAnalytical chemistryGeneral Materials ScienceX ray irradiationCondensed Matter PhysicsLuminescencebusinessRadiation Effects and Defects in Solids
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Phase formation in mixed TiO2-ZrO2 oxides prepared by sol-gel method

2011

Pure titania, zirconia, and mixed oxides (3—37 mol.% of ZrO2) are prepared using the sol-gel method and calcined at different temperatures. The calcined samples are characterized by Raman spectroscopy, X-ray powder diffraction, scanning electron microscopy, transmission electron microscopy, and nitrogen adsorption porosimetry. Measurements reveal a thermal stability of the titania anatase phase that slightly increases in the presence of 3—13 mol.% of zirconia. Practically, the titania anatase-rutile phase transformation is hindered during the temperature increase above 700 C. The mixed oxide with 37 mol.% of ZrO2 treated at 550 C shows a new single amorphous phase with a surface area of the…

Anatasex ray scatteringMaterials scienceelectron microscopyScanning electron microscopeMineralogysrilankite Rietveld method.Inorganic Chemistryx ray scattering; electron microscopyChemical engineeringTransmission electron microscopyPhase (matter)Materials ChemistryMixed oxideTiO2—ZrO2 mixed oxidesol-gel methodCubic zirconiaPhysical and Theoretical ChemistryPowder diffractionSol-gelSettore CHIM/02 - Chimica Fisica
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X-ray computed tomography investigations of Cucuteni ceramic statuettes:

2013

Deciphering the internal structure of prehistoric artefacts can provide spectacular insights that might help us understand the people who made them. In order to preserve the integrity of these relics of past civilisations, it is desirable to make such investigations using non-destructive techniques. Recent decades have witnessed a growth in the X-ray computed tomography (CT) applications in the study of cultural heritage objects. This paper presents and discusses tomographic investigations of two Cucuteni ceramic statuettes discovered in Romania. The study was made with a CT device specially designed for archaeometric applications.

ArcheologyEngineeringmedicine.diagnostic_testbusiness.industryComputed tomographyceramicsX-ray Computed TomographyArchaeologyCultural heritageX ray computedAnthropologyCucutenistatuettesmedicinelcsh:ArchaeologyTomographylcsh:CC1-960business
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XMM observations of NGC 2516 stars

2007

We present the characteristics of the X-ray variability of stars in the cluster NGC 2516 as derived from XMM-Newton/EPIC/pn data. The X-ray variations on short (hours), medium (months), and long (years) time scales have been explored. We detected 303 distinct X-ray sources by analysing six EPIC/pn observations; 194 of them are members of the cluster. Stars of all spectral types, from the early-types to the late-M dwarfs, were detected. Cone search capability for table J/A+A/456/977/table2 (X-ray and optical properties of NGC 2516 members in the XMM-Newton/EPIC/pn observations having more than 25 counts.)

Astrophysics and AstronomyAstrophysics::High Energy Astrophysical PhenomenaPhysicsAstrophysics::Cosmology and Extragalactic AstrophysicsLate type starsX-ray sourcesstellar astronomyOptical astronomyCosmologyOpen star clustersPhotometryobservational astronomyX ray sourcesAstrophysics::Solar and Stellar AstrophysicsWide-band photometryNatural SciencesLate-type starsAstrophysics::Galaxy AstrophysicsInfrared photometryWide band photometry
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XMM spectroscopy of TWA 5

2006

We present results of X-ray spectroscopy for TWA 5, a member of the young TW Hydrae association, observed with XMM-Newton. TWA 5 is a multiple system which shows H{alpha} emission, a signature typical of classical T Tauri stars, but no infrared excess. From this analysis of the RGS and EPIC spectra, we have derived the emission measure distribution vs. temperature of the X-ray emitting plasma, its abundances, and the electron density.

Astrophysics and AstronomyAstrophysics::High Energy Astrophysical PhenomenaPhysicsAstrophysics::Cosmology and Extragalactic AstrophysicsX-ray sourcesobservational astronomyPre main sequence starsX ray sourcesStellar AstronomyAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsPre-main sequence starsMultiple starsNatural SciencescosmologyAstrophysics::Galaxy AstrophysicsSpectroscopy
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XMM-Newton survey of two Upper Scorpius regions

2007

We studied X-ray emission from young stars by analyzing the deep XMM-Newton observations of two regions of the Upper Scorpius association with an age of 5Myr. Based on near infrared and optical photometry we identified 22 Upper Scorpius photometric members among the 224 detected X-ray sources. We derived coronal properties of Upper Scorpius stars by performing X-ray spectral and timing analyses. The study of four strong and isolated stellar flares allowed us to derive the length of the flaring loops. Cone search capability for table J/A+A/459/199/tableb1 (Sources detected in the CTIO observations) Cone search capability for table J/A+A/459/199/tablec1 (Sources detected in the Danish 1.54m o…

Astrophysics and AstronomyAstrophysics::High Energy Astrophysical PhenomenaPhysicsAstrophysics::Cosmology and Extragalactic AstrophysicsX-ray sourcesstellar astronomyOptical astronomyCosmologyPhotometryobservational astronomyPre main sequence starsX ray sourcesAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsWide-band photometryPre-main sequence starsNatural SciencesAstrophysics::Galaxy AstrophysicsInfrared photometryWide band photometry
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Old MS stars in young moving groups

2009

The associations and moving groups of young stars are excellent laboratories to investigate the stellar formation in the solar neighborhood. Past results confirmed that a non-negligible fraction of old main-sequence stars is present in the lists of members of the young stellar kinematic groups. A detailed study on the properties of these samples is needed to separate the young stars from old main-sequence stars with similar space motion, in order to identify the origin of these structures. Our intention is to characterize the sample of stars members of the young moving groups and determine their age distribution to quantify the contamination by old main-sequence stars, in particular, in the…

Astrophysics and AstronomyPhysicsAstrophysics::Cosmology and Extragalactic AstrophysicsX-ray sourcesobservational astronomyPhotometryX ray sourcesStellar AstronomyDwarf starsAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsNatural SciencescosmologyAstrophysics::Galaxy AstrophysicsInfrared photometry
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Star formation region NGC 6530

2005

We present astrometry and BVI photometry, down to V~22, of the very young open cluster NGC 6530, obtained from observations taken with the Wide Field Imager camera at the MPG/ESO 2.2m Telescope. We have positionally matched our optical catalog with the list of X-ray sources found in a Chandra-ACIS observation, finding a total of 828 common stars, 90% of which are pre-main sequence stars in NGC 6530. Cone search capability for table J/A+A/430/941/table4 (Cross-identifications of this catalog with the previous works of Walker (1957ApJ...125..636W), Kilambi (1977MNRAS.178..423K) and Sung et al. (2000, Cat. )) Cone search capability for table J/A+A/430/941/table5 (Cross-identifications of the o…

Astrophysics and AstronomyPhysicsX-ray sourcesstellar astronomyOptical astronomyCosmologyOpen star clustersPhotometryobservational astronomyPre main sequence starsX ray sourcesWide-band photometryPre-main sequence starsNatural SciencesInfrared photometryWide band photometry
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XMM-Newton Extended Survey of Taurus

2007

The XMM-Newton Extended Survey of the Taurus Molecular Cloud (XEST) surveys the most populated ~5 square degrees of the Taurus Molecular Cloud, using the XMM-Newton X-ray observatory to study the thermal structure, variability, and long-term evolution of hot plasma, to investigate the magnetic dynamo, and to search for new potential members of the association. We present overall correlations with fundamental stellar parameters that were derived from the previous literature. The present overview paper introduces the project and provides the basic results from the X-ray analysis of all sources detected in the XEST survey. Comprehensive tables summarize the stellar properties of all targets su…

Astrophysics and AstronomyStellar associationsPhysicsAstrophysics::High Energy Astrophysical PhenomenaAstrophysics::Instrumentation and Methods for AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsSurveysX-ray sourcesComputer Science::Digital Librariesobservational astronomyPre main sequence starsX ray sourcesStellar AstronomyAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsNatural SciencesPre-main sequence starscosmologyAstrophysics::Galaxy Astrophysics
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