Search results for "MAI"

showing 10 items of 6279 documents

Students’ Perceptions of Family Entrepreneurship – A Study on Family Business Academic Education

2010

L’objectif de cette recherche est d’analyser les points de vue d’étudiants universitaires envers la condition des entrepreneurs. Le fond théorique analyse l’interaction entre l’entreprise familiale, le propriétaireship, et l’éducation sur la condition des entrepreneurs. 211 étudiants de l’Université de Jyväskylä ont participé à cette étude pendant le cours fondamental de Basic business studies appelé “Introduction to Entrepreneurship and Business Operations” en septembre 2007. 143 d’entre eux ont écrit un essai d’une page, soit en finnois soit en anglais, sur les entreprises familiales et les propriétaires familiales. Les étudiants ont écrit sur le phénomène avec leurs propres mots. Les rés…

Academic educationEntrepreneurshipSocial Sciences and Humanitiesfamily businesscontent analysiseducación en iniciativa empresarialéducation de la condition des entrepreneurspedagogyFamily businessGeneral Medicineentreprise familialeanalyse de content.Political sciencepédagogieempresa familiarEthnologySciences Humaines et SocialesHumanitiespedagogía análisis de contenidosentrepreneurship educationManagement international
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Molecular mechanisms of endomembrane trafficking in plants

2021

Abstract Endomembrane trafficking is essential for all eukaryotic cells. The best-characterized membrane trafficking organelles include the endoplasmic reticulum (ER), Golgi apparatus, early and recycling endosomes, multivesicular body, or late endosome, lysosome/vacuole, and plasma membrane. Although historically plants have given rise to cell biology, our understanding of membrane trafficking has mainly been shaped by the much more studied mammalian and yeast models. Whereas organelles and major protein families that regulate endomembrane trafficking are largely conserved across all eukaryotes, exciting variations are emerging from advances in plant cell biology research. In this review, …

AcademicSubjects/SCI01280EndosomeENDOPLASMIC-RETICULUMGolgi ApparatusPlant ScienceSUSPENSION-CULTURED CELLSBiologyDOMAIN-CONTAINING PROTEINSEndoplasmic ReticulumEndocytosissymbols.namesakeLysosomeAutophagymedicineEndomembrane systemVACUOLAR TRAFFICKINGPlant Physiological PhenomenaLate endosomeAcademicSubjects/SCI01270AcademicSubjects/SCI02288AcademicSubjects/SCI02287Endoplasmic reticulumAcademicSubjects/SCI02286AutophagyBiology and Life SciencesBiological TransportRETICULUM EXPORT SITESCell BiologyGolgi apparatusCLATHRIN-MEDIATED ENDOCYTOSISEndocytosisFocus on Cell BiologyCell biologyTRANS-GOLGI NETWORKEditorialmedicine.anatomical_structureP24 FAMILY PROTEINSMEMBRANE TRAFFICKINGPLASMA-MEMBRANEVacuolessymbolsThe Plant Cell
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Optimal Damping Constant Investigation on a Quarter-Car

2013

This paper shows an investigation on optimal damping constant performed in the frequency domain. The optimal damping constant is meant as that value that minimizes the acceleration of all connected bodies characterizing a two degree of freedom system sketching a quarter car. The connected bodies are sprung and unsprung mass respectively for quarter of chassis and tire, this last keeps the contact with the ground and it is connected with the sprung mass through a shock absorber characterized by spring and fluid damper. Optimal damping constant was determined by imposing analytical conditions on the expression of acceleration of two masses. Afterwards, the variation of acceleration and positi…

AccelerationShock absorberChassisSpring (device)Frequency domainMathematical analysisSprung massUnsprung massMathematicsDamper
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The N-terminal domain of the light-harvesting chlorophyll a/b-binding protein complex (LHCII) is essential for its acclimative proteolysis.

2000

AbstractVariations in the amount of the light-harvesting chlorophyll a/b-binding protein complex (LHCII) is essential for regulation of the uptake of light into photosystem II. An endogenous proteolytic system was found to be involved in the degradation of LHCII in response to elevated light intensities and the proteolysis was shown to be under tight regulation [Yang, D.-H. et al. (1998) Plant Physiol. 118, 827–834]. In this study, the substrate specificity and recognition site towards the protease were examined using reconstituted wild-type and mutant recombinant LHCII. The results show that the LHCII apoprotein and the monomeric form of the holoprotein are targeted for proteolysis while t…

Acclimative proteaseChlorophyll aN-terminal domainPhotosystem IImedicine.medical_treatmentProteolysisMutantMolecular Sequence DataPhotosynthetic Reaction Center Complex ProteinsBiophysicsLight-Harvesting Protein ComplexesRecognition siteEndogenyLight-harvesting complex IIBiochemistrylaw.inventionchemistry.chemical_compoundStructural BiologylawSpinacia oleraceaGeneticsmedicineAmino Acid SequenceMolecular BiologyProteasemedicine.diagnostic_testSequence Homology Amino AcidChemistryBinding proteinHydrolysisPhotosystem II Protein ComplexCell BiologyBiochemistryRecombinant light-harvesting complex IIProteolysisRecombinant DNAFEBS letters
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The self-perceived commitment and relationship maintenance behaviors among Finnish-Chinese couples in Finland : an application of the investment mode…

2015

The investment model (2003) has been widely used in romantic relationship studies but rarely in an intercultural context. This study tests the investment model by examining Finnish-Chinese couples’ self-perceptions of commitment level and relationship maintenance behaviors. A qualitative research method with deductive thematic analysis approach is applied. This study finds that Finnish-Chinese couples have relatively high level of commitment. They tend to remain in their relationships, to actively derogate alternatives, to sacrifice self-welfare for gratifying relationship well-being, to perceive their relationships as good and healthy and to choose relationship constructive responses under…

AccommodationparisuhdeInvestment ModelCommitmentRelationship Maintenance Behaviorssuomalaisetsitoutuminenkulttuurienvälinen viestintäDevelopmentkiinalaisetIntercultural CouplesNegotiationkulttuurienvälisyys
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X-rays from accretion shocks in classical T Tauri stars: 2D MHD modeling and the role of local absorption

2013

AbstractIn classical T Tauri stars (CTTS) strong shocks are formed where the accretion funnel impacts with the denser stellar chromosphere. Although current models of accretion provide a plausible global picture of this process, some fundamental aspects are still unclear: the observed X-ray luminosity in accretion shocks is order of magnitudes lower than predicted; the observed density and temperature structures of the hot post-shock region are puzzling and still unexplained by models.To address these issues we performed 2D MHD simulations describing an accretion stream impacting onto the chromosphere of a CTTS, exploring different configurations and strengths of the magnetic field. From th…

Accretion MHD Stars: pre-main sequence X-rays: starsPhysicsbusiness.product_categoryAstronomyAstronomy and AstrophysicsAstrophysicsViewing angleAccretion (astrophysics)Spectral lineMagnetic fieldT Tauri starSettore FIS/05 - Astronomia E AstrofisicaSpace and Planetary Sciencepre-main sequence X-rays: stars [Accretion MHD Stars]FunnelMagnetohydrodynamicsbusinessChromosphereProceedings of the International Astronomical Union
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UV variability and accretion dynamics in the young open cluster NGC 2264

2015

We explore UV and optical variability signatures for several hundred members of NGC 2264 (3 Myr). We performed simultaneous u- and r-band monitoring over two full weeks with CFHT/MegaCam. About 750 young stars are probed; 40% of them are accreting. Statistically distinct variability properties are observed for accreting and non-accreting cluster members. The accretors exhibit a significantly higher level of variability than the non-accretors, especially in the UV. The amount of u-band variability correlates statistically with UV excess in disk-bearing objects, which suggests that accretion and star-disk interaction are the main sources of variability. Cool magnetic spots, several hundred de…

AccretionAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsSettore FIS/05 - Astronomia E AstrofisicaStars: low-maAstrophysics::Solar and Stellar Astrophysicsaccretion diskAstrophysics::Galaxy AstrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Stars: variables: T TauriPhysicsPhotosphereHerbig Ae/BeAstronomy and AstrophysicsAstronomy and AstrophysicUltraviolet: starAccretion (astrophysics)StarsWavelengthAmplitudeAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceOpen clusters and associations: individual: NGC 2264Stars: pre-main sequenceAstrophysics::Earth and Planetary AstrophysicsOpen cluster
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X-shooter spectroscopy of young stars with disks. The TW Hydrae association as a probe of the final stages of disk accretion

2019

We investigate ongoing accretion activity in young stars in the TW Hydrae association (TWA, ~8-10 Myr), an ideal target to probe the final stages of disk accretion down to brown dwarf masses. Our sample comprises eleven TWA members with infrared excess, amounting to 85% of the total TWA population with disks, with spectral types between M0 and M9, and masses between 0.58 and 0.02 Msol. We employed homogeneous spectroscopic data from 300 to 2500 nm, obtained with X-shooter, to derive individual extinction, stellar parameters, and accretion parameters simultaneously. We then examined Balmer lines and forbidden emission lines to probe the physics of the star-disk interaction environment. We de…

AccretionOpen clusters and associations: individual: TWA010504 meteorology & atmospheric sciencesBrown dwarfFOS: Physical sciencesTechniques: spectroscopicAstrophysicsProtoplanetary diskStellar classification01 natural sciencesspectroscopic [Techniques]symbols.namesakeSettore FIS/05 - Astronomia E Astrofisicalow-mass [Stars]pre-main sequence [Stars]0103 physical sciencesStars: low-maTW HydraeQB Astronomy010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)QC0105 earth and related environmental sciencesQBEarth and Planetary Astrophysics (astro-ph.EP)PhysicsInfrared excessBalmer seriesAstronomy and AstrophysicsDASAstrophysics - Astrophysics of GalaxiesAccretion (astrophysics)StarsQC PhysicsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceAccretion diskAstrophysics of Galaxies (astro-ph.GA)Accretion diskssymbolsStars: pre-main sequenceindividual: TWA [Open clusters and associations]Astrophysics - Earth and Planetary Astrophysics
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UV And X-Ray Emission from Impacts of Fragmented Accretion Streams on Classical T Tauri Stars

2016

According to the magnetoshperic accretion scenario, during their evo- lution, Classical T Tauri stars accrete material from their circumstellar disk. The accretion process is regulated by the stellar magnetic eld and produces hot and dense post-shocks on the stellar surface as a result of impacts of the downfalling material. The impact regions are expected to strongly radiate in UV and X-rays. Several lines of evidence support the magnetospheric accretion scenario, especially in optical and infrared bands. However several points still remain unclear as, for instance,where the complex-pro le UV lines originate, or whether and how UV and X-ray emission is produced in the same shock region. Th…

AccretionPlasmaSettore FIS/05 - Astronomia E AstrofisicaAccretion accretion disks Stars: pre-main sequence Stars: variables: T Tauri Herbig Ae/BeT Tauri StarsdiskMagnetohydrodinamicMHD simulation
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Redshifted X-rays from the material accreting onto TW Hya: evidence of a low-latitude accretion spot

2017

High resolution spectroscopy, providing constraints on plasma motions and temperatures, is a powerful means to investigate the structure of accretion streams in CTTS. In particular, the accretion shock region, where the accreting material is heated to temperatures of a few MK as it continues its inward bulk motion, can be probed by X-ray spectroscopy. To attempt to detect for the first time the motion of this X-ray-emitting post-shock material, we searched for a Doppler shift in the deep Chandra/HETGS observation of the CTTS TW Hya. This test should unveil the nature of this X-ray emitting plasma component in CTTS, and constrain the accretion stream geometry. We searched for a Doppler shift…

AccretionTechniques: spectroscopicFOS: Physical sciencesAstrophysics01 natural sciencesSettore FIS/05 - Astronomia E Astrofisica0103 physical sciencesTW HydraeX-rays: starEmission spectrumSpectroscopy010303 astronomy & astrophysicsStars: variables: T TauriSolar and Stellar Astrophysics (astro-ph.SR)PhysicsPhotosphereLine-of-sight010308 nuclear & particles physicsHerbig Ae/BeAstronomy and AstrophysicsAstronomy and AstrophysicRedshiftAccretion (astrophysics)T Tauri starAstrophysics - Solar and Stellar AstrophysicsAccretion diskSpace and Planetary ScienceStars: pre-main sequence
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