Search results for "49"

showing 10 items of 1208 documents

New corological and biological data of the Red Gum Lerp Psyllid, Glycaspis brimblecombei Moore, 1964 in Italy (Hemiptera, Psyllidae)

2011

Glycaspis brimblecombei Moore, 1964 is a psyllid (Hemiptera: Psyllidae) pest of Eucalyptus, native toAustralia and first recorded in Europe: Spain in 2008 and more recently (2010) in Italy. The present paper dealswith recent research, carried out in central Italy, with new data on the distribution and biology of this species.

HemipteraPsyllidaeItalylcsh:QH540-549.5lcsh:Botanylcsh:Zoologynew recordslcsh:Ecologylcsh:QL1-991lcsh:QK1-989Biodiversity Journal
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Marx en la Sociología

2018

Hernàndez i DobonUNESCO::SOCIOLOGÍA1137-7038 8537 Arxius de sociologia 493757 2018 38 6508340 Marx en la Sociología Herzog:SOCIOLOGÍA [UNESCO]BennoFrancesc Jesús 5 8
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[Llistat de compra i donacions de llibres fets per Roque Francés, Luis Exarque, Mariano Hernández i Vicente Salvá]

Ms Títol donat pel catalogador

Hernández Mariano Donacions i llegatsSalvá Vicente 1786-1849 Donacions i llegatsFrancés Roque Donacions i llegatsExarque Luis Donacions i llegatsUniversitat de València. Biblioteca Històrica Inventaris
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Outflows and spectral evolution in the eclipsing AMXP SWIFT J1749.4–2807 with NICER, XMM-Newton, and NuSTAR

2022

The neutron star low-mass X-ray binary SWIFT J1749.4–2807 is the only known eclipsing accreting millisecond X-ray pulsar. In this manuscript, we perform a spectral characterization of the system throughout its 2021, 2-week-long outburst, analysing 11 NICER observations and quasi-simultaneous XMM-Newton and NuSTAR single observations at the outburst peak. The broad-band spectrum is well-modelled with a blackbody component with a temperature of ∼0.6 keV, most likely consistent with a hotspot on the neutron star surface, and a Comptonization spectrum with power-law index Γ ∼ 1.9, arising from a hot corona at ∼12 keV. No direct emission from the disc was found, possibly due to it being too cool…

High Energy Astrophysical Phenomena (astro-ph.HE)Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and AstrophysicsX-rays: individuals: Swift J1749.4-2807accretion discsStars: neutronX-rays: binariesSettore FIS/05 - Astronomia E AstrofisicaaccretionAccretion accretion discs[SDU]Sciences of the Universe [physics]Space and Planetary ScienceAstrophysics::Solar and Stellar AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaMonthly Notices of the Royal Astronomical Society
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Overionization in X-ray spectra: a new paradigm for Mixed-Morphology SNRs

2011

Mixed-morphology SNRs are characterized by a shell-like radio emission, a centrally peaked X-ray morphology, and by interaction with molecular clouds. Many models have been proposed to explain these peculiar remnants, but their physical origin is still unclear. The recent discovery of over-ionized (i. e. recombining) ejecta in 3 mixed-morphology SNRs has dramatically challenged all the previous models and opened up new, unexpected scenarios. I review the main properties of these remnants and their peculiar X-ray spectral properties. I also discuss the hydrodynamic model developed to explain the presence of over-ionized ejecta in W49B and present a list of open issues that still need to be c…

High Energy Astrophysical Phenomena (astro-ph.HE)Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics - High Energy Astrophysical PhenomenaMixed-morphology SNRs are characterized by a shell-like radio emission a centrally peaked X-ray morphology and by interaction with molecular clouds. Many models have been proposed to explain these peculiar remnants but their physical origin is still unclear. The recent discovery of overionized (i. e. recombining) ejecta in 3 mixed-morphology SNRs has dramatically challenged all the previous models and opened up new unexpected scenarios. I review the main properties of these remnants and their peculiar X-ray spectral properties. I also discuss the hydrodynamic model developed to explain the presence of overionized ejecta in W49B and present a list of open issues that still need to be clarified.Astrophysics::Galaxy Astrophysics
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Unveiling the spatial structure of the overionized plasma in the supernova remnant W49B

2011

W49B is a mixed-morphology supernova remnant with thermal X-ray emission dominated by the ejecta. In this remnant, the presence of overionized plasma has been directly established, with information about its spatial structure. However, the physical origin of the overionized plasma in W49B has not yet been understood. We investigate this intriguing issue through a 2D hydrodynamic model that takes into account, for the first time, the mixing of ejecta with the inhomogeneous circumstellar and interstellar medium, the thermal conduction, the radiative losses from optically thin plasma, and the deviations from equilibrium of ionization induced by plasma dynamics. The model was set up on the basi…

High Energy Astrophysical Phenomena (astro-ph.HE)ISM: individual objects: W49BPhysics::Plasma PhysicsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics - High Energy Astrophysical PhenomenaISM: individual objects: G43.3-0.2Astrophysics::Galaxy Astrophysicshydrodynamicmethods: numericalISM: supernova remnants
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The discovery of the 401 Hz accreting millisecond pulsar IGR J17498-2921 in a 3.8 h orbit

2011

We report on the detection of a 400.99018734(1) Hz coherent signal in the Rossi X-ray Timing Explorer light curves of the recently discovered X-ray transient, IGR J17498-2921. By analysing the frequency modulation caused by the orbital motion observed between August 13 and September 8, 2011, we derive an orbital solution for the binary system with a period of 3.8432275(3) hr. The measured mass function, f(M_2, M_1, i)=0.00203807(8) Msun, allows to set a lower limit of 0.17 Msun on the mass of the companion star, while an upper limit of 0.48 Msun is set by imposing that the companion star does not overfill its Roche lobe. We observe a marginally significant evolution of the signal frequency …

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsLight curveSpectral lineNeutron starOrbitSettore FIS/05 - Astronomia E AstrofisicaSpace and Planetary ScienceMillisecond pulsarOrbital motionAstrophysics::Solar and Stellar AstrophysicsRoche lobeAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomenaneutron stars: rotation pulsars: individual:IGR J17498-2921 X-rays: binaries [stars]stars: neutron stars: rotation pulsars: individual:IGR J17498-2921 X-rays: binariesNoise (radio)
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Spatial identification of the overionized plasma in W49B

2010

Recent Suzaku X-ray observations of the ejecta-dominated supernova remnant W49B have shown that in the global spectrum there is a clear indication for the presence of overionized plasma whose physical origin is still under debate. In order to ascertain the physical origin of such a rapidly cooling plasma, we focus on the study of its spatial localization within the X-ray emitting ejecta. We confirm the presence of a saw-edged excess (interpreted as a strong radiative recombination continuum) in the global spectrum above 8 keV, emerging above the ionization-equilibrium model. We produce a hardness ratio map to determine where the plasma is overionized and we perform a spectral analysis of th…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsHardness ratioAstrophysics::High Energy Astrophysical PhenomenaInterstellar cloudFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsPlasmaX-rays: ISM ISM: supernova remnants ISM: individual object: W49BSettore FIS/05 - Astronomia E AstrofisicaSpace and Planetary ScienceSpontaneous emissionSpectral analysisSpatial localizationAstrophysics - High Energy Astrophysical PhenomenaEjectaSupernova remnantISM ISM: supernova remnants ISM: individual object: W49B [X-rays]Astrophysics::Galaxy Astrophysics
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Belief in God, Confidence in the Church and Secularization in Scandinavia

2021

We used the three latest rounds of the religion module of International Social Survey Programme to study secularization in Denmark, Norway, and Sweden, focusing on belief in God. We restricted our sample to the affiliated with the majority Protestant churches and the unaffiliated and analyzed the trends toward disaffiliation and disbelief in God. Then, we studied the association between confidence in churches, religious/secular upbringing, and demographic controls with belief in God using multinomial logistic regression models. Our treatment of belief in God as a nominal variable allowed the inclusion of both the element of doubt and different images of God in the analyses. The trends towar…

HistorySociology and Political ScienceDenmarkchurchInternational Social Survey ProgrammeBL1-2790Sociology & anthropologyProtestantismbelief in godBelief in GodSociologyGlaubeNorwegenfaithConceptualizationNorwaySkandinavienAttendanceDänemarkReligion III - ISSP 2008 (ZA4950 v2.3.0); International Social Survey Programme: Religion IV - ISSP 2018 (ZA7570 v2.1.0); multinomial logistic regression [Religious and Moral Pluralism (RAMP) (ZA3170 v1.1.0); International Social Survey Programme]ProtestantismusRegressionReligionreligiöse SozialisationScandinaviaddc:301confidenceconfidence in churchesSocial psychologyBelief in God; Confidence in Churches; Religious Socialization; Secularization; Scandinavian countries; Multinomial logistic regressionVertrauenContext (language use)secularizationGender StudiesPower (social and political)Secularizationscandinavian countriesSociology; Religion; SecularizationSwedenReligionssoziologieGottReligions. Mythology. RationalismVDP::Humaniora: 000::Teologi og religionsvitenskap: 150ISSPReligious studiesSäkularisierungPhilosophyProtestantismSoziologie AnthropologieAnthropologygodreligious socializationSociology of ReligionKirchemultinomial logistic regressionSchweden
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Observacion hecha por el Dr. Gregorio Marcìa, Medico, y Cirujano de esta Ciudad de Valencia, Demostrador pùblico de Cirugia en ella, y Socio de la Re…

1749

Caplletra ornada Sign.: [ ]4 Reclams

Històries clíniques Godella (Comunitat Valenciana 1749 Obres anteriors a 1800Històries clíniques Godella (Comunitat Valenciana 1749 Obres anteriors al 1800Medicina clinica Estudi de casos Godella (Comunitat Valenciana) 1749 Obres anteriors a 1800Medicina clinica Estudi de casos Godella (Comunitat Valenciana) 1749 Obres anteriors al 1800
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