Search results for "mna"

showing 10 items of 1167 documents

Diving below the spin-down limit: Constraints on gravitational waves from the energetic young pulsar PSR J0537-6910

2021

We present a search for continuous gravitational-wave signals from the young, energetic X-ray pulsar PSR J0537-6910 using data from the second and third observing runs of LIGO and Virgo. The search is enabled by a contemporaneous timing ephemeris obtained using NICER data. The NICER ephemeris has also been extended through 2020 October and includes three new glitches. PSR J0537-6910 has the largest spin-down luminosity of any pulsar and is highly active with regards to glitches. Analyses of its long-term and inter-glitch braking indices provided intriguing evidence that its spin-down energy budget may include gravitational-wave emission from a time-varying mass quadrupole moment. Its 62 Hz …

010504 meteorology & atmospheric sciencesAstronomyAstrophysicsEP/ T017325/101 natural sciencesrotationGeneral Relativity and Quantum CosmologyPSR J0537−6910neutron starsLuminosityGravitatational Waves PSR J0537−6910 LIGO VirgoHISTORYLIGOSupernova remnantneutron star010303 astronomy & astrophysicsgravitational waveQCQBpulsarPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Settore FIS/03N157BPhysics/dk/atira/pure/sustainabledevelopmentgoals/partnershipsGravitational waves neutron stars pulsarEPSRCPhysical Sciencesmoment: multipole[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Astrophysics - High Energy Astrophysical PhenomenaGravitational wavedata analysis methodPSR J0537-6910Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astronomy & AstrophysicsEphemeris1ST SEARCHGravitational wavesX-raySDG 17 - Partnerships for the GoalsPulsar0103 physical sciences/dk/atira/pure/subjectarea/asjc/1900/1912X-ray: emissiongravitational waves; pulsars; PSR J0537-6910; neutron starsSTFCAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesScience & TechnologyNeutron Star Interior Composition ExplorerR-MODEGravitational waveVirgopulsar: rotationRCUKAstronomy and AstrophysicsLIGONeutron starVIRGOSUPERNOVA REMNANTSpace and Planetary Sciencegravitational radiation: emissionpulsars/dk/atira/pure/subjectarea/asjc/3100/3103Gravitatational Waves[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Detection of X-ray flares from AX J1714.1-3912, the unidentified source near RX J1713.7-3946

2018

Molecular clouds are predicted to emit nonthermal X-rays when they are close to particle-accelerating supernova remnants (SNRs), and the hard X-ray source AX J1714.1-3912, near the SNR RX J1713.7-3946, has long been considered a candidate for diffuse nonthermal emission associated with cosmic rays diffusing from the remnant to a closeby molecular cloud. We aim at ascertaining the nature of this source by analyzing two dedicated X-ray observations performed with Suzaku and Chandra. We extracted images from the data in various energy bands, spectra, and light curves and studied the long-term evolution of the X-ray emission on the basis of the ~4.5 yr time separation between the two observatio…

010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayContext (language use)Astrophysics01 natural sciencesSpectral lineX-rays: binariesSettore FIS/05 - Astronomia E Astrofisica0103 physical sciencesX-rays: bursts010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsISM: supernova remnants0105 earth and related environmental sciencesHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsMolecular cloudAstronomy and AstrophysicsLight curveX-rays: ISMSupernovaOrders of magnitude (time)Space and Planetary ScienceSupergiantAstrophysics - High Energy Astrophysical Phenomena
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XMM-Newton observation of the supernova remnant Kes 78 (G32.8-0.1): Evidence for shock-cloud interaction

2017

The Galactic supernova remnant Kes 78 is surrounded by dense molecular clouds, whose projected position overlaps with the extended HESS gamma-ray source HESS J1852-000. The X-ray emission from the remnant has been recently revealed by Suzaku observations, which have shown indications for a hard X-ray component in the spectra, possibly associated with synchrotron radiation. We aim at describing the spatial distribution of the physical properties of the X-ray emitting plasma and at revealing the effects of the interaction of the remnant with the inhomogeneous ambient medium. We also aim at investigating the origin of the gamma-ray emission, which may be Inverse Compton radiation associated wi…

010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaHadronSynchrotron radiationFOS: Physical sciencesElectronAstrophysicsISM: individual objects: Kes 7801 natural sciencesSpectral linelaw.inventionlawISM: cloud0103 physical sciencesSupernova remnant010303 astronomy & astrophysicsISM: supernova remnantAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Molecular cloudAstronomy and AstrophysicsPlasmaAstronomy and AstrophysicAcceleration of particleSynchrotronX-rays: ISM13. Climate actionSpace and Planetary ScienceAstrophysics - High Energy Astrophysical Phenomena
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Deep XMM-Newton Observations Reveal the Origin of Recombining Plasma in the Supernova Remnant W44

2019

Recent X-ray studies revealed over-ionized recombining plasmas (RPs) in a dozen mixed-morphology (MM) supernova remnants (SNRs). However, the physical process of the over-ionization has not been fully understood yet. Here we report on spatially resolved spectroscopy of X-ray emission from W44, one of the over-ionized MM-SNRs, using XMM-Newton data from deep observations, aiming to clarify the physical origin of the over-ionization. We find that combination of low electron temperature and low recombination timescale is achieved in the region interacting with dense molecular clouds. Moreover, a clear anti-correlation between the electron temperature and the recombining timescale is obtained f…

010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaSupernova remnants (1667)FOS: Physical sciencesAstrophysicsMolecular cloud01 natural sciencesX-ray astronomySettore FIS/05 - Astronomia E AstrofisicaPlasma astrophysics (1261)Supernova remnant0103 physical sciencesPlasma astrophysicsSupernova remnantAdiabatic processSpectroscopy010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsX-ray astronomyMolecular cloudAstronomy and AstrophysicsPlasmaSupernovaSpace and Planetary ScienceMolecular clouds (1072)Electron temperatureX-ray astronomy (1810)Astrophysics - High Energy Astrophysical PhenomenaThe Astrophysical Journal
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Indication of a Pulsar Wind Nebula in the Hard X-Ray Emission from SN 1987A

2021

Since the day of its explosion, SN 1987A (SN87A) was closely monitored with the aim to study its evolution and to detect its central compact relic. The detection of neutrinos from the supernova strongly supports the formation of a neutron star (NS). However, the constant and fruitless search for this object has led to different hypotheses on its nature. Up to date, the detection in the ALMA data of a feature somehow compatible with the emission arising from a proto Pulsar Wind Nebula (PWN) is the only hint of the existence of such elusive compact object. Here we tackle this 33-years old issue by analyzing archived observations of SN87A performed Chandra and NuSTAR in different years. We fir…

010504 meteorology & atmospheric sciencesSupernova remnantsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesSynchrotron radiationAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsCompact starX-ray sources01 natural sciencesPulsar wind nebulaNeutron starsX-ray astronomy0103 physical sciencesPlasma astrophysicsEjectaX-ray point sources010303 astronomy & astrophysicsCompact objectsX-ray observatoriesShocksAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsX-ray astronomyAstronomy and AstrophysicsNeutron starSupernovaInterstellar synchrotron emissionSpace and Planetary ScienceNeutrinoAstrophysics - High Energy Astrophysical Phenomena
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The problem of misidentification between edible and poisonous wild plants: Reports from the Mediterranean area

2018

Abstract Today, in many European countries, people are looking for wild edible plants to experience new tastes and flavors, by following the new trend of being green and environmentally friendly. Young borage and spinach leaves can be easily confused by inexpert pickers with those of other plants, including poisonous ones, such as Mandragora autumnalis Bertol. (mandrake) or Digitalis purpurea L. (foxglove), common in southern and northern Italy respectively. In the last twenty years, several cases of intoxication by accidental ingestion of mandrake and foxglove have been reported. The purpose of this work was to perform a pharmacognostic characterization of young leaves from borage, mandrak…

0106 biological sciences0301 basic medicineChromatography GasDigitalis GlycosidePhytochemicalsIntoxicationBiologyPhytochemicalToxicology010603 evolutionary biology01 natural sciencesEdible plantGas Chromatography-Mass SpectrometryAccidental ingestion03 medical and health sciencesPlant leaveAlkaloidsAlkaloidHumansDiscriminant analysePoisonous plants Edible plants Plant leaves Accidental ingestion Intoxication Discriminant analysesBorageTraditional medicineMediterranean RegionSettore BIO/02 - Botanica SistematicaDigitalis purpureafood and beveragesMandragora autumnalisDigitalis GlycosidesDiscriminant analysesGeneral MedicineMandrakebiology.organism_classificationPoisonous plantPlant LeavesPlants Toxic030104 developmental biologyPhytochemicalItalyChromatography GaPoisonous plantsSettore BIO/03 - Botanica Ambientale E ApplicataAccidental ingestionEdible plantsEdible plantsMediterranean areaPlants EdibleFood ScienceHuman
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Application of high resolution melting assay (HRM) to study temperature-dependent intraspecific competition in a pathogenic bacterium

2017

AbstractStudies on species’ responses to climate change have focused largely on the direct effect of abiotic factors and in particular temperature, neglecting the effects of biotic interactions in determining the outcome of climate change projections. Many microbes rely on strong interference competition; hence the fitness of many pathogenic bacteria could be a function of both their growth properties and intraspecific competition. However, due to technical challenges in distinguishing and tracking individual strains, experimental evidence on intraspecific competition has been limited so far. Here, we developed a robust application of the high-resolution melting (HRM) assay to study head-to…

0106 biological sciences0301 basic medicineGenotypeClimate ChangeScienceintraspecific competitionmedia_common.quotation_subject030106 microbiologyZoologymedicine.disease_causeFlavobacterium010603 evolutionary biology01 natural sciencesArticleCompetition (biology)Intraspecific competitionHigh Resolution Melt03 medical and health sciencesmedicineAnimalsmedia_commonAbiotic componentMultidisciplinarybiologyStrain (chemistry)EcologyQFishesTemperatureRpathogenic bacteriaPathogenic bacteriabiology.organism_classificationhigh-resolution melting (HRM) assay13. Climate actionFlavobacterium columnareMedicinelämpötilaGenetic FitnessBacteriaScientific Reports
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2021

Environmental heterogeneity is a central component influencing the virulence and epidemiology of infectious diseases. The number and distribution of susceptible hosts determines disease transmission opportunities, shifting the epidemiological threshold between the spread and fadeout of a disease. Similarly, the presence and diversity of other hosts, pathogens and environmental microbes, may inhibit or accelerate an epidemic. This has important applied implications in farming environments, where high numbers of susceptible hosts are maintained in conditions of minimal environmental heterogeneity. We investigated how the quantity and quality of aquaculture enrichments (few vs. many stones; cl…

0106 biological sciences0301 basic medicineMicrobiology (medical)VirulenceDisease010603 evolutionary biology01 natural sciencesBiochemistryMicrobiology03 medical and health sciencesAquaculturePharmacology (medical)General Pharmacology Toxicology and PharmaceuticsPathogen2. Zero hungerbiologyEcologybusiness.industryTransmission (medicine)Host (biology)biology.organism_classification030104 developmental biologyInfectious DiseasesAgricultureFlavobacterium columnarebusinessAntibiotics
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2019

Hosts are typically infected with multiple strains or genotypes of one or several parasite species. These infections can take place simultaneously, but also at different times, i.e. sequentially, when one of the parasites establishes first. Sequential parasite dynamics are common in nature, but also in intensive farming units such as aquaculture. However, knowledge of effects of previous exposures on virulence of current infections in intensive farming is very limited. This is critical as consecutive epidemics and infection history of a host could underlie failures in management practices and medical intervention of diseases. Here, we explored effects of timing of multiple infections on vir…

0106 biological sciences0301 basic medicineeducation.field_of_studybiologybusiness.industryHost (biology)PopulationVirulenceZoologyDiseasebiology.organism_classification010603 evolutionary biology01 natural sciences03 medical and health sciences030104 developmental biologyAquacultureDisease management (agriculture)Flavobacterium columnareGeneticsParasite hostingGeneral Agricultural and Biological SciencesbusinesseducationEcology Evolution Behavior and SystematicsEvolutionary Applications
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Broad thermal tolerance is negatively correlated with virulence in an opportunistic bacterial pathogen

2018

Predicting the effects of global increase in temperatures on disease virulence is challenging, especially for environmental opportunistic bacteria, because pathogen fitness may be differentially affected by temperature within and outside host environment. So far, there is very little empirical evidence on the connections between optimal temperature range and virulence in environmentally growing pathogens. Here, we explored whether the virulence of an environmentally growing opportunistic fish pathogen, Flavobacterium columnare, is malleable to evolutionary changes via correlated selection on thermal tolerance. To this end, we experimentally quantified the thermal performance curves (TPCs) f…

0106 biological sciences0301 basic medicinelämmönsietoGrowing seasonVirulenceZoology010603 evolutionary biology01 natural sciencesthermal tolerancethermal performance curvesbakteerit03 medical and health sciencesOpportunistic pathogenGeneticsPathogenEcology Evolution Behavior and Systematics2. Zero hungerGenetic diversitybiologyHost (biology)opportunistic pathogenta1182virulenssiOriginal Articlesilmastonmuutoksetbiology.organism_classificationvirulenceclimate changetaudinaiheuttajat030104 developmental biology13. Climate actionFlavobacterium columnareta1181Original ArticleGeneral Agricultural and Biological SciencesBacteriaEvolutionary Applications
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