Search results for "Dwarf"

showing 10 items of 136 documents

XIPE: the X-ray imaging polarimetry explorer

2013

arXiv:1309.6995v1.-- et al.

AstronomyAstrophysics::High Energy Astrophysical PhenomenaPolarimetryFOS: Physical sciencesAstrophysics7. Clean energy01 natural scienceslaw.inventionX-raySettore FIS/05 - Astronomia E Astrofisicalaw0103 physical sciencesPolarimetry010303 astronomy & astrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Solar and Stellar Astrophysics (astro-ph.SR)Astronomy X-ray PolarimetryPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Solar flare[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]White dwarfAstronomy and AstrophysicsTorusMagnetic reconnectionPolarization (waves)Neutron starAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary Science[SDU]Sciences of the Universe [physics]Astrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsFlare
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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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XMM-Newton detection of the 2.1 ms coherent pulsations from IGR J17379-3747

2018

We report on the detection of X-ray pulsations at 2.1 ms from the known X-ray burster IGR J17379-3747 using XMM-Newton. The coherent signal shows a clear Doppler modulation from which we estimate an orbital period of ~1.9 hours and a projected semi-major axis of ~8 lt-ms. Taking into account the lack of eclipses (inclination angle of < 75 deg) and assuming a neutron star mass of 1.4 Msun, we estimated a minimum companion star of ~0.06 Msun. Considerations on the probability distribution of the binary inclination angle make less likely the hypothesis of a main-sequence companion star. On the other hand, the close correspondence with the orbital parameters of the accreting millisecond puls…

Astrophysics::High Energy Astrophysical PhenomenaBrown dwarfFOS: Physical sciencesgeneral; stars: neutron; X-rays: binaries; accretion accretion disks [binaries]AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsEphemeris01 natural sciencesstars: neutronSettore FIS/05 - Astronomia E AstrofisicaMillisecond pulsar0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsEmission spectrum010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsOrbital elementsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)accretion accretion disksAccretion (meteorology)010308 nuclear & particles physicsAstronomy and AstrophysicsOrbital periodX-rays: binarieNeutron starbinaries: generalSpace and Planetary ScienceAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomena
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The clinical and molecular spectrum of QRICH1 associated neurodevelopmental disorder

2022

De novo variants in QRICH1 (Glutamine-rich protein 1) has recently been reported in 11 individuals with intellectual disability. The function of QRICH1 is largely unknown but it is likely to play a key role in the unfolded response of endoplasmic reticulum (ER) stress through transcriptional control of proteostasis. In this study, we present 27 additional individuals and delineate the clinical and molecular spectrum of the individuals (n=38) with QRICH1 variants. The main clinical features were mild to moderate developmental delay/intellectual disability (71%), non-specific facial dysmorphism (92%) and hypotonia (39%). Additional findings included poor weight gain (29%), short stature (29%)…

Autism Spectrum Disorder[SDV]Life Sciences [q-bio]DwarfismBiologyBioinformaticsWeight GainShort stature03 medical and health sciences0302 clinical medicineNeurodevelopmental disorderNeuroimagingSeizuresvariable expressivityIntellectual disabilityGeneticsmedicineMissense mutationHumansQRICH1hypotoniaGenetics (clinical)030304 developmental biology0303 health sciencesmedicine.diseaseQRICH1Hypotoniashort statureScoliosisvariantAutism spectrum disorderNeurodevelopmental Disordersintellectual disabilityMuscle Hypotoniamedicine.symptom030217 neurology & neurosurgery
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Reduction in insulin sensitivity and inadequate β-cell capacity to counteract the increase in insulin resistance in children with idiopathic growth h…

2014

Purpose: To evaluate the performance of various indexes of insulin sensitivity and secretion and to identify the most useful indicator of deterioration of glucose metabolism in a cohort of children with growth hormone (GH) deficiency (GHD) during GH treatment. Methods: In 73 GHD children (55 M, 18 F; mean age 10.5 years) at baseline and after 12 months of treatment, we evaluated a number of surrogate indexes of insulin secretion and sensitivity. In a subgroup of 11 children we also performed an euglycemic hyperinsulinemic clamp. Results: After 12 months, a significant increase in fasting glucose (p < 0.001) and HbA1c levels (p < 0.001) was documented, despite all children remained with a no…

Blood GlucoseMalemedicine.medical_specialtyAdolescentHormone Replacement TherapyEndocrinology Diabetes and Metabolismmedicine.medical_treatmentChildren; Glucose metabolism; Growth hormone treatment; Insulin secretion; Insulin sensitivity; Endocrinology Diabetes and Metabolism; EndocrinologyHypopituitarismCarbohydrate metabolismHypopituitarismSettore MED/13 - EndocrinologiaEndocrinologyInsulin resistanceInsulin-Secreting CellsInternal medicinemedicineHormone replacement therapy (male-to-female)HumansInsulinGrowth hormone treatmentChildDwarfism PituitaryChildrenGlucose metabolismGlucose tolerance testmedicine.diagnostic_testHuman Growth Hormonebusiness.industryInsulin secretionInsulinGlucose Tolerance TestInsulin sensitivitymedicine.diseaseGrowth hormone treatmentTreatment OutcomeEndocrinologyChild PreschoolConcomitantFemaleInsulin Resistancebusiness
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One-hour post-load plasma glucose level is associated with a worse metabolic profile in children with GH deficiency

2017

Purpose: In children, the plasma glucose value at 1 h (1hPG) during OGTT higher than 132.5 mg/dl is a predictor of alterations in glucose metabolism. We aimed to metabolically characterize GHD children according to 1hPG levels. Methods: Fifty-one GHD children (35 M, 16 F; mean age 8.6 years), grouped according to 1hPG, were evaluated at diagnosis and after 12 months of GH treatment (GHT) and compared with 50 matched controls at baseline. Auxological parameters, insulin-like growth factor-1 (IGF-1), glucose and insulin during OGTT, lipid profile, the oral disposition index (DIo), the homeostasis model assessment estimate of insulin resistance (Homa-IR), and the insulin sensitivity index (ISI…

Blood GlucoseMalemedicine.medical_specialtyTime FactorsTime FactorEndocrinology Diabetes and Metabolismmedicine.medical_treatment030209 endocrinology & metabolism030204 cardiovascular system & hematologyCarbohydrate metabolismSettore MED/13 - Endocrinologia03 medical and health scienceschemistry.chemical_compound0302 clinical medicineEndocrinologyInsulin resistanceGH treatmentInternal medicineInsulin SecretionHumansInsulinMedicineChildDwarfism PituitaryGrowth hormoneGlucose tolerance testmedicine.diagnostic_testHuman Growth Hormonebusiness.industryCholesterolInsulinCase-control studynutritional and metabolic diseasesGlucose Tolerance TestInsulin sensitivitymedicine.diseaseMetabolismEndocrinologychemistryCase-Control StudiesChild PreschoolMetabolomeFemaleInsulin ResistanceCase-Control StudiebusinessLipid profileHomeostasisHumanJournal of Endocrinological Investigation
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A brown dwarf orbiting an M-dwarf:MOA 2009-BLG-411L

2012

Context. Caustic crossing is the clearest signature of binary lenses in microlensing. In the present context, this signature is diluted by the large source star but a detailed analysis has allowed the companion signal to be extracted.Aims. MOA 2009-BLG-411 was detected on August 5, 2009 by the MOA-Collaboration. Alerted as a high-magnification event, it was sensitive to planets. Suspected anomalies in the light curve were not confirmed by a real-time model, but further analysis revealed small deviations from a single lens extended source fit.Methods. Thanks to observations by all the collaborations, this event was well monitored. We first decided to characterize the source star properties b…

Brown dwarfContext (language use)Astrophysicsgravitational lensing: microAstrophysics::Cosmology and Extragalactic AstrophysicsGravitational microlensing01 natural sciencesSettore FIS/05 - Astronomia e AstrofisicaPlanet0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsstars: individual: MOA 2009-BLG-411L010308 nuclear & particles physicsAstronomyMOA 2009-BLG-411L; gravitational lensing; starsAstronomy and AstrophysicsRadiusLight curveGalaxyGravitational lensbinaries: generalSpace and Planetary ScienceAstrophysics::Earth and Planetary Astrophysicsbinaries: general; gravitational lensing: micro; stars: individual: MOA 2009-BLG-411L
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MILES extended: Stellar population synthesis models from the optical to the infrared

2016

We present the first single-burst stellar population models which covers the optical and the infrared wavelength range between 3500 and 50000 Angstrom and which are exclusively based on empirical stellar spectra. To obtain these joint models, we combined the extended MILES models in the optical with our new infrared models that are based on the IRTF (Infrared Telescope Facility) library. The latter are available only for a limited range in terms of both age and metallicity. Our combined single-burst stellar population models were calculated for ages larger than 1 Gyr, for metallicities between [Fe/H] = -0.40 and 0.26, for initial mass functions of various types and slopes, and on the basis …

CAII TRIPLETStellar populationInfraredMetallicityINITIAL MASS FUNCTIONBROWN DWARFSInfrared telescopeFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesAstronomical spectroscopyinfrared: galaxiesATMOSPHERIC PARAMETERS0103 physical sciencesRange (statistics)Astrophysics::Solar and Stellar Astrophysics2.5 MU-MGIANT BRANCH STARS010303 astronomy & astrophysicsinfrared: starsEMPIRICAL CALIBRATIONAstrophysics::Galaxy AstrophysicsPhysics010308 nuclear & particles physicsNear-infrared spectroscopyHIGH-SPECTRAL-RESOLUTIONAstronomy and AstrophysicsEVOLUTIONARY SYNTHESISAstrophysics - Astrophysics of GalaxiesGalaxySpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)NEWTON-TELESCOPE LIBRARYgalaxies: stellar contentAstrophysics::Earth and Planetary Astrophysics
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Expression of PIP1 and PIP2 aquaporins is enhanced in olive dwarf genotypes and is related to root and leaf hydraulic conductance

2007

The expression of OePIP1.1 and OePIP2.1 aquaporins in root, stem and leaf was higher in Olea europaea L. (olive) plants carrying a dwarfing (D) clone as rootstock, than in plants carrying a vigorous (M) clone as rootstock. The highest difference of expression between plants with D and M rootstocks was detected in the root and for the PIP2 gene, the transcripts of which show a high water channel activity in oocytes.  Compared with plants with M rootstock, plants with D rootstock showed reduced root and canopy biomass and reduced hydraulic conductance of the bulk root system (Kroot). Hydraulic conductance of D roots was higher than that of M roots when Kroot was scaled by root DW, in agreemen…

Canopyhydraulic conductancePhysiologyshootAquaporindroughtPlant ScienceRoot systemembolismAquaporin; water channel; cavitation; drought; embolism; olive; hydraulic conductance; shoot; water stress; compensatory mechanism.olivewater stresscavitationGene expressionBotanyGeneticsbiologyAquaporinfungifood and beverageswater channelCell BiologyGeneral Medicinebiology.organism_classificationGraftingDwarfingcompensatory mechanismOleaRootstockPhysiologia Plantarum
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Stellar hydrodynamics with glaister's riemann solver: An approach to the stellar collapse

1990

La resolution de Remann approximee de la solution des equations d'Euler de la dynamique des gaz 1 D, developpee par Glaister P. (1988, J. Comput. Phys., 74) est introduite dans un code hydrodynamique lagrangien et appliquee a l'effondrement stellaire a symetrie spherique

Cauchy problemPhysicsNumerical AnalysisPhysics and Astronomy (miscellaneous)Applied MathematicsWhite dwarfGas dynamicsRiemann solverComputer Science ApplicationsComputational MathematicsSupernovasymbols.namesakeClassical mechanicsModeling and SimulationGravitational collapsesymbolsCircular symmetryStellar evolutionJournal of Computational Physics
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