Search results for "33"

showing 10 items of 1917 documents

Economic Feasibility of Measures for Energy Efficiency

2014

In this chapter the economic impact of some measures for energy efficiency, both using automation of technical infrastructures (according to EN 15232) as well as implementing passive measures concerning the use of building materials and techniques (according to EN 15271), is studied. The chapter is organized as follows. First, a technical-economical study on the evaluation of the impact on residential buildings of Building Automation Control, BAC, and Technical Building Management, TBM, systems is presented. Then the same assessment of some passive measures that can be employed is carried out using the Passive House Standard for Mediterranean warm climates is shown. Numerical elaborations h…

Architectural engineeringbusiness.industrySample (statistics)Load profileSettore ING-IND/33 - Sistemi Elettrici Per L'EnergiaBAC and TBMbuilding automationEnvironmental sciencemedia_common.cataloged_instanceEconomic impact analysisPassive houseEuropean unionbusinessBuilding managementenergy efficiencymedia_commonBuilding automationEfficient energy use
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Espositione di tutti i vocaboli, et luoghi difficili, che nel Libro si trouano : Con vna brieue dimostratione di molte comparationi [et] sentenze del…

1549

Sig. *8, **6 Retrat d'Ariosto al verso de la port. - Capital grav Reclams al final de cada quadern

Ariosto Lodovico 1474-1533 Crítica i interpretació Obres anteriors al 1800Literatura italiana S.XVI Obres anteriors al 1800
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Macroscopic expressions of molecular adiabatic compressibility of methyl and ethyl caprate under high pressure and high temperature

2014

The molecular compressibility, which is a macroscopic quantity to reveal the microcompressibility by additivity of molecular constitutions, is considered as a fixed value for specific organic liquids. In this study, we introduced two calculated expressions of molecular adiabatic compressibility to demonstrate its pressure and temperature dependency. The first one was developed from Wada’s constant expression based on experimental data of density and sound velocity. Secondly, by introducing the 2D fitting expressions and their partial derivative of pressure and temperature, molecular compressibility dependency was analyzed further, and a 3D fitting expression was obtained from the calculated…

Article SubjectApplied Mathematicslcsh:MathematicsThermodynamicsFunction (mathematics)Analysis; Applied Mathematicslcsh:QA1-939VDP::Mathematics and natural science: 400::Physics: 430::Atomic physics molecular physics: 433Consistency (statistics)Additive functionRange (statistics)CompressibilityPartial derivativeCompressibility factorConstant (mathematics)AnalysisMathematics
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"Table 37" of "Energy dependence of event shapes and of alpha(s) at LEP-2."

1999

Distributions of the Total Jet Broadening (BSUM) at cm energies 133, 161 and 172 GeV.

Astrophysics::High Energy Astrophysical PhenomenaE+ E- --> HADRONSE+ E- --> JETSE+ E- ScatteringExclusiveHigh Energy Physics::ExperimentDN/DBSUMSingle Differential DistributionJet ProductionNuclear Experiment133.0-172.0
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"Table 23" of "Energy dependence of event shapes and of alpha(s) at LEP-2."

1999

Distributions of Planarity at cm energies 133, 161 and 172 GeV.

Astrophysics::High Energy Astrophysical PhenomenaE+ E- --> HADRONSE+ E- --> JETSE+ E- ScatteringExclusiveHigh Energy Physics::ExperimentSingle Differential DistributionJet ProductionComputer Science::Computational GeometryNuclear ExperimentDN/DPLANARITY133.0-172.0
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"Table 21" of "Energy dependence of event shapes and of alpha(s) at LEP-2."

1999

Distributions of Sphericity at cm energies 133, 161 and 172 GeV.

Astrophysics::High Energy Astrophysical PhenomenaE+ E- --> HADRONSE+ E- --> JETSE+ E- ScatteringExclusiveHigh Energy Physics::ExperimentSingle Differential DistributionJet ProductionNuclear Experiment133.0-172.0DN/DSPHERICITY
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Indications of non-conservative mass-transfer in AMXPs

2019

Context. Since the discovery of the first Accreting Millisecond X-ray Pulsar SAX J1808.4-3658 in 1998, the family of these sources kept growing on. Currently, it counts 22 members. All AMXPs are transients with usually very long quiescence periods, implying that mass accretion rate in these systems is quite low and not constant. Moreover, for at least three sources, a non-conservative evolution was also proposed. Aims. Our purpose is to study the long term averaged mass-accretion rates in all the Accreting Millisecond X-ray Pulsars discovered so far, to investigate a non-conservative mass-transfer scenario. Methods. We calculated the expected mass-transfer rate under the hypothesis of a con…

Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesContext (language use)X-rays: starsAstrophysicsCompact star01 natural sciencesLuminositystars: neutronX-rays: binariesPulsarpulsars: general0103 physical sciencesX-rays: individuals: IGR J17498−2921X-rays: individuals: IGR J17498-2921010303 astronomy & astrophysicsX-rays: individuals: XTE J1814−338PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Accretion (meteorology)010308 nuclear & particles physicsGravitational waveAstronomy and AstrophysicsX-rays: binarieX-rays: individuals: XTE J1814-338Radiation pressureSpace and Planetary ScienceAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Magnetic dipole
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Correlated X-ray spectral and timing variability of the Be/X-ray binary V0332+53/BQ Camelopardalis during a type II outburst

2005

We have used INTEGRAL & RXTE data to investigate the timing properties of the source in correlation with its spectral states as defined by different positions in the colour-colour diagram. The source shows two distinct branches in the colour-colour diagram that resemble those of the Z sources. The hard branch (similar to the horizontal branch of Z sources) is characterised by a low-amplitude change of the hard colour compared to the change in the soft colour. In the soft branch (analogue to the normal branch) the amplitude of variability of the hard colour is about three times larger than that of the soft colour. As the count rate decreases the source moves up gradually through the soft…

Astrophysics::High Energy Astrophysical PhenomenaPhase (waves)X-ray binaryFOS: Physical sciencesFluxAstrophysicsAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICABinary starsPulsarStars ; Individual star ; V0332+54 ; BQ Cam ; X-rays ; Binary stars ; Neutron – stars: binaries: close –stars: emission line BeX-raysBQ CamPhysicsAstrophysics (astro-ph)Astronomy and AstrophysicsHorizontal branchStars:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]Neutron starAmplitudeSpace and Planetary ScienceV0332+54binaries: close –stars: emission line Be [Neutron – stars]Individual starUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniaNoise (radio):ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
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Black-Hole Accretion Discs and Jets at Super-Eddington Luminosity

2004

Super-Eddington accretion discs with 3 and 15 dot M_E around black holes with mass 10 M_sun are examined by two-dimensional radiation hydrodynamical calculations extending from the inner disc edge to 5*10^4 r_g and lasting up to \sim 10^6 r_g/c. The dominant radiation-pressure force in the inner region of the disc accelerates the gas vertically to the disc plane, and jets with 0.2 -- 0.4$c$ are formed along the rotational axis. In the case of the lower accretion rate, the initially anisotropic high-velocity jet expands outward and becomes gradually isotropic flow in the distant region. The mass-outflow rate from the outer boundary is as large as \sim 10^{19} -- 10^{23} g s^{-1}, but it is v…

Astrophysics::High Energy Astrophysical Phenomenablack hole physicsAstrophysics (astro-ph)SS 433FOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsaccretion discsthermalradiation mechanismsaccretionhydrodynamicsX-raysindividualAstrophysics::Galaxy Astrophysics
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Cannabinoid CB1 receptor activation modulates spontaneous contractile activity in mouse ileal longitudinal muscle.

2007

The purpose of the present study was to examine whether cannabinoid receptor agonists influence spontaneous contractile activity of longitudinal muscle in mouse ileum in vitro. Isolated segments of mouse ileum displayed spontaneous contractions with an amplitude and frequency of about 300 mg and 30 cpm, respectively. The endocannabinoid anandamide (1-100 microM), the selective cannabinoid CB(1) receptor agonist, ACEA (0.1 microM-10 microM), but not the selective cannabinoid CB(2) receptor agonist, JWH 133 (0.1 microM-10 microM), reduced in a concentration-dependent manner the spontaneous mechanical activity. The inhibitory effect consisted in a decrease of the mean amplitude of longitudinal…

AtropineMaleAgonistmedicine.medical_specialtyCB1 receptorIndolesCannabinoid receptorPolyunsaturated Alkamidesmedicine.drug_classmedicine.medical_treatmentMouse ileumArachidonic AcidsTetrodotoxinIn Vitro TechniquesDepolarization-induced suppression of inhibitionHexamethoniumReceptor Cannabinoid CB2Micechemistry.chemical_compoundPiperidinesReceptor Cannabinoid CB1IleumInternal medicineCannabinoid Receptor ModulatorsmedicineAnimalsCannabinoidPharmacologyDose-Response Relationship DrugCannabinoidsChemistryMuscle SmoothCannabinoid Receptor AgonistsReceptor antagonistEndocannabinoid systemAcetylcholineMice Inbred C57BLNG-Nitroarginine Methyl EsterEndocrinologyApaminJWH-133PyrazolesCannabinoidRimonabantSpontaneous mechanical activityEndocannabinoidsMuscle Contraction
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