Search results for "raga"

showing 10 items of 1852 documents

Phytochemical profile and insecticidal activity of Drimia pancration (Asparagaceae) against adults of Stegobium paniceum (Anobiidae)

2020

Chemical and spectroscopic investigation of the bulbs of Drimia pancration resulted in the isolation of one known flavonol (1), never isolated from this plant species, and of three previously described steroidal saponins (2–4), but whose configuration at their stereogenic centres was not clearly determined. By mean of 1H NMR, 13C NMR, nuclear overhauser effects (NOE) and two-dimensional NMR spectra the full stereochemical structures of compounds 2–4 were proved and all the 1H and 13C signals were assigned. Furthermore, the methanol and butanol extracts of D. pancration were tested against adults of Stegobium paniceum beetles. Despite the non-significant results regarding the repellent activ…

Drimiasteroidal saponinsflavonolStegobium paniceumbiologyTraditional medicine010405 organic chemistryOrganic ChemistryinsecticideSettore CHIM/06 - Chimica OrganicaPlant Sciencebiology.organism_classification01 natural sciencesBiochemistry0104 chemical sciencesAnalytical Chemistry010404 medicinal & biomolecular chemistryAsparagaceaeAnobiidaePhytochemicalDrimia pancrationPlant speciesSettore BIO/15 - Biologia Farmaceutica
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Spectroscopic properties of pure and Coumarin 153-doped thin films of sol-gel silica xerogels

1999

Abstract Thin-films doped with Coumarin 153, an important laser dye, have been prepared by the sol-gel method. Spectroscopic properties of the entrapped dye are studied by electronic absorption, diffuse reflectance, electronic excitation, emission and time-resolved emission techniques. The obtained results indicate that the entrapment of the dye results in formation of molecular aggregates having absorption and emission characteristics different from those of the monomeric dye. The blue matrix emission band (at approx. 450 nm) is relatively short-lived while the red band (at approx. 700 nm) displays a very long lifetime. Electronic excitation spectra of the sol-gel thin-films suggest that t…

Dye laserChemistryOrganic ChemistryDopingAnalytical chemistryPhysics::OpticsAstrophysics::Cosmology and Extragalactic AstrophysicsAnalytical ChemistryInorganic ChemistryDiffuse reflectionAbsorption (chemistry)Thin filmLuminescenceAstrophysics::Galaxy AstrophysicsSpectroscopyExcitationSol-gelJournal of Molecular Structure
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"Table 1" of "Measurements of the line shape of the Z0 and determination of electroweak parameters from its hadronic and leptonic decays"

1994

Hadronic cross sections from the 1990 data set. Additional systematic uncertainties come from efficiencies and background of 0.4 pct in addition to the luminosity uncertainty 0.7 pct.

E+ E- --> HADRONSE+ E- --> Z0E+ E- ScatteringIntegrated Cross SectionExclusiveHigh Energy Physics::ExperimentAstrophysics::Cosmology and Extragalactic AstrophysicsCross SectionR measurementSIG88.223-94.202Astrophysics::Galaxy Astrophysics
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"Table 40" of "Tuning and test of fragmentation models based on identified particles and precision event shape data."

1996

Compilation of multiplicities of baryons from current LEP I data.

E+ E- --> LAMBDA XE+ E- --> SIGMA(1385P13)- XE+ E- --> SIGMA(1385P13)+ XStrange productionNuclear TheoryHigh Energy Physics::PhenomenologyE+ E- --> OMEGA- X91.2Astrophysics::Cosmology and Extragalactic AstrophysicsE+ E- --> P XMULTInclusiveE+ E- --> XI(1530P13)0 XE+ E- --> DELTA(1232P33)++ XE+ E- ScatteringComputer Science::Programming LanguagesE+ E- --> XI- XHigh Energy Physics::ExperimentE+ E- --> LAMBDA/B0 X
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"Table 10" of "Cross-sections and leptonic forward-backward asymmetries from the Z0 running of LEP."

2000

Cross section and forward-backward asymmetry in the TAU+ TAU- channel for the 1993 data. Additional systematic error for cross section of 0.60 PCT (efficiencies and backgrounds) and 0.29 PCT (absolute luminosity). Additional systematic error for the asymmetry of 0.0020.

E+ E- --> TAU+ TAU-Asymmetry MeasurementE+ E- ScatteringIntegrated Cross SectionExclusiveHigh Energy Physics::ExperimentAstrophysics::Cosmology and Extragalactic Astrophysics89.431-93.015Cross SectionTau productionSIGASYM
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IPHAS-selected classical Be stars

2016

We present a semi-automatic procedure to obtain fundamental physical parameters and distances of classical Be (CBe) stars, based on the Barbier-Chalonge-Divan (BCD) spectrophotometric system. Our aim is to apply this procedure to a large sample of CBe stars detected by the IPHAS photometric survey, to determine their fundamental physical parameters and to explore their suitability as galactic structure tracers. In this paper we describe the methodology used and the validation of the procedure by comparing our results with those obtained from different independent astrophysical techniques for subsamples of stars in common with other studies. We also present a test case study of the galactic …

Early type starsAstrophysics and AstronomyPhysicsAstrophysics::Instrumentation and Methods for AstrophysicsStellar distanceAstrophysics::Cosmology and Extragalactic AstrophysicsComputer Science::Digital Librariesobservational astronomyStellar AstronomyEarly-type starsBe starsAstrophysics::Solar and Stellar AstrophysicsNatural SciencesAstrophysics::Galaxy Astrophysics
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Be stars in the exofield of CoRoT. II.

2018

The class of Be stars are the epitome of rapid rotators in the main sequence. These stars are privileged candidates for studying the incidence of rotation on the stellar internal structure and on non-radial pulsations. Pulsations are considered possible mechanisms to trigger mass-ejection phenomena required to build up the circumstellar disks of Be stars. Time series analyses of the light curves of 15 faint Be stars observed with the CoRoT satellite were performed to obtain the distribution of non-radial pulsation (NRP) frequencies in their power spectra at epochs with and without light outbursts and to discriminate pulsations from rotation-related photometric variations. Standard Fourier t…

Early type starsAstrophysics and AstronomyStellar AstronomyEarly-type starsBe starsPhysicsAstrophysics::High Energy Astrophysical PhenomenaAstrophysics::Instrumentation and Methods for AstrophysicsAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsNatural SciencesAstrophysics::Galaxy Astrophysics
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Non-thermal processes in coronae and beyond

2012

This contribution summarizes the splinter session "Non-thermal processes in coronae and beyond" held at the Cool Stars 17 workshop in Barcelona in 2012. It covers new developments in high energy non-thermal effects in the Earth's exosphere, solar and stellar flares, the diffuse emission in star forming regions and reviews the state and the challenges of the underlying atomic databases.

Earth and Planetary Astrophysics (astro-ph.EP)High Energy Astrophysical Phenomena (astro-ph.HE)Sun: flareMethods: laboratoryStars: flareFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstronomy and AstrophysicAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary SciencePhysics::Space PhysicsAstrophysics::Solar and Stellar AstrophysicsRadiation mechanism: non-thermalAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaAtomic dataAstrophysics::Galaxy AstrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics - Earth and Planetary Astrophysics
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Hiding in plain sight: observing planet-starspot crossings with the James Webb Space Telescope

2021

Transiting exoplanets orbiting active stars frequently occult starspots and faculae on the visible stellar disc. Such occultations are often rejected from spectrophotometric transits, as it is assumed they do not contain relevant information for the study of exoplanet atmopsheres. However, they can provide useful constraints to retrieve the temperature of active features and their effect on transmission spectra. We analyse the capabilities of the James Webb Space Telescope in the determination of the spectra of occulted starspots, despite its lack of optical wavelength instruments on board. Focusing on K and M spectral types, we simulate starspots with different temperatures and in differen…

Earth and Planetary Astrophysics (astro-ph.EP)PhysicsJames Webb Space TelescopeStarspotAstrophysics::Instrumentation and Methods for AstrophysicsFOS: Physical sciencesAstronomyAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsStellar classificationExoplanetStarsWavelengthAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary SciencePlanetAstrophysics::Solar and Stellar AstrophysicsPrismAstrophysics::Earth and Planetary AstrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsAstrophysics - Earth and Planetary Astrophysics
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PROBING THE DARK MATTER RADIAL PROFILE IN LENS GALAXIES AND THE SIZE OF X-RAY EMITTING REGION IN QUASARS WITH MICROLENSING

2015

We use X-ray and optical microlensing measurements to study the shape of the dark matter density profile in the lens galaxies and the size of the (soft) X-ray emission region. We show that single epoch X-ray microlensing is sensitive to the source size. Our results, in good agreement with previous estimates, show that the size of the X-ray emission region scales roughly linearly with the black hole mass, with a half-light radius of where . This corresponds to a size of or ?1 lt-day for a black hole mass of . We simultaneously estimated the fraction of the local surface mass density in stars, finding that the stellar mass fraction is ? = 0.20 ? 0.05 at an average radius of , where Re is the …

Effective radiusPhysicsStellar massAstrophysics::High Energy Astrophysical PhenomenaDark matterAstronomy and AstrophysicsQuasarAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsGravitational microlensingGalaxyBlack holeStarsSpace and Planetary ScienceAstrophysics::Earth and Planetary AstrophysicsAstrophysics::Galaxy AstrophysicsThe Astrophysical Journal
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