Search results for " shock"

showing 10 items of 691 documents

Exosomal Hsp60 in human colon cancer

2014

Heat shock proteincolon cancerExtracellular vescicle
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Protective role of heat shock proteins in Parkinson's disease.

2010

Parkinson’s disease (PD) is the second most common neurodegenerative disease after Alzheimer’s disease. Despite a large amount of research, the pathogenetic mechanism of these diseases has not yet been clarified. Abnormal protein folding, oxidative stress, mitochondrial dysfunction, and apoptotic mechanisms have all been reported as causes of neurodegenerative diseases in association with neuroinflammatory mechanisms which, by generating deleterious molecules, could promote the cascade of events leading to neurodegeneration. Heat shock proteins (HSPs) play a central role in preventing protein misfolding and inhibiting apoptotic activity, and represent a class of proteins potentially involve…

Heat shock proteins Parkinson disease neuroprotective roleParkinson's diseasebiologyNeurodegenerationParkinson DiseaseDiseasemedicine.diseasemedicine.disease_causeHsp90Hsp70PathogenesisNeurologyHeat shock proteinImmunologymedicinebiology.proteinAnimalsHumansHSP70 Heat-Shock ProteinsNeurology (clinical)HSP90 Heat-Shock ProteinsNeuroscienceOxidative stressHeat-Shock ProteinsNeuro-degenerative diseases
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Role of heme oxygenase-1 (HSP32) and HSP90 in glioblastoma

2017

Glioblastoma (GBM) is the most common and malignant primary brain tumor in adults. The current treatment regimes for glioblastoma demonstrated a low efficiency and offer a poor prognosis. Advancements in conventional treatment strategies have only yielded modest improvements in overall survival. The heat shockproteins, heme oxygenase-1 (HO-1) and Hsp90, serve these pivotal roles in tumor cells and have been identified as effective targets for developing therapeutics. This topic review summarizes the current preclinical and clinical evidences and rationale to define the potential of HO-1 and Hsp90 in GBM progression and chemoresistance.

Heme oxygenaseMolecular chaperonesHeat shock proteinHsp90GlioblastomaCancer
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Sequence-Specific Repression of Cotranslational Translocation of the Hepatitis B Virus Envelope Proteins Coincides with Binding of Heat Shock Protein…

1997

AbstractThe large L envelope protein of the hepatitis B virus has the peculiar capacity to adopt two transmembrane topologies. The N-terminal preS domain of L initially remains in the cytosol while the S domain is cotranslationally inserted into the endoplasmic reticulum membrane. The preS region of about half of the L molecules is posttranslationally translocated to the lumenal space. We now demonstrate that the repression of cotranslational translocation of preS is conferred by a preS1-specific sequence. By analysis of L deletion mutants, the cytosolic anchorage determinant was mapped to amino acid sequence 70 to 94 of L. The intrinsic potential of this determinant to suppress cotranslati…

Hepatitis B virusHSC70 Heat-Shock ProteinsRecombinant Fusion ProteinsPlasma protein bindingBiologyGenes envCytosolViral Envelope ProteinsHeat shock proteinVirologyHumansHSP70 Heat-Shock ProteinsBinding sitePromoter Regions GeneticPeptide sequenceBinding SitesBase SequenceCell-Free SystemEndoplasmic reticulumHSC70 Heat-Shock ProteinsOligonucleotides AntisenseMolecular biologyTransmembrane proteinChaperone (protein)Protein Biosynthesisbiology.proteinMutagenesis Site-DirectedMetallothioneinCarrier ProteinsProtein BindingVirology
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Expression of the 60 kDa heat shock protein in normal and inflamed liver.

1993

The 60 kDa heat shock proteins (HSP 60) have been well conserved throughout evolution and are highly immunogenic. Cross-reactivity between bacterial and mammalian HSP 60 is considered a likely mechanism in the pathogenesis of autoimmune diseases. T cell and B cell reactivity to HSP 60 is found in patients with rheumatoid or juvenile arthritis, and the expression of HSP 60 in the inflamed joint is found to be increased. In this study the presence of HSP 60 was demonstrated in normal and inflamed lives. HSP 60 was found to be predominantly expressed in hepatocytes and Kupffer cells, and mainly localized in mitochondria. Heat stress in the form of a 1 h incubation at 42 degrees C increased HSP…

HepatitisHepatologyT cellKupffer cellInflammationAutoimmune hepatitisChaperonin 60Biologymedicine.diseaseMolecular biologyHepatitisPathogenesismedicine.anatomical_structureLiverReference ValuesHeat shock proteinImmunologyChronic DiseasemedicineHumansmedicine.symptomB cellHeat-Shock ProteinsJournal of hepatology
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XMM-Newton Large Program on SN1006 - I: Methods and Initial Results of Spatially-Resolved Spectroscopy

2015

Based on our newly developed methods and the XMM-Newton large program of SN1006, we extract and analyze the spectra from 3596 tessellated regions of this SNR each with 0.3-8 keV counts $>10^4$. For the first time, we map out multiple physical parameters, such as the temperature ($kT$), electron density ($n_e$), ionization parameter ($n_et$), ionization age ($t_{ion}$), metal abundances, as well as the radio-to-X-ray slope ($\alpha$) and cutoff frequency ($\nu_{cutoff}$) of the synchrotron emission. We construct probability distribution functions of $kT$ and $n_et$, and model them with several Gaussians, in order to characterize the average thermal and ionization states of such an extended s…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsElectron densityAstrophysics::High Energy Astrophysical Phenomenadata analysis cosmic rays ISM: supernova remnants X-rays: ISM [acceleration of particles shock waves methods]FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysicsacceleration of particles shock waves methods: data analysis cosmic rays ISM: supernova remnants X-rays: ISMSpectral lineInterstellar mediumSupernovaSpace and Planetary ScienceIonizationAstrophysics::Solar and Stellar AstrophysicsSpectroscopySupernova remnantAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Equivalent widthAstrophysics::Galaxy Astrophysics
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On the observability of T Tauri accretion shocks in the X-ray band

2010

Context. High resolution X-ray observations of classical T Tauri stars (CTTSs) show a soft X-ray excess due to high density plasma (n_e=10^11-10^13 cm^-3). This emission has been attributed to shock-heated accreting material impacting onto the stellar surface. Aims. We investigate the observability of the shock-heated accreting material in the X-ray band as a function of the accretion stream properties (velocity, density, and metal abundance) in the case of plasma-beta<<1 in the post-shock zone. Methods. We use a 1-D hydrodynamic model describing the impact of an accretion stream onto the chromosphere, including the effects of radiative cooling, gravity and thermal conduction. We expl…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsRadiative coolingAstrophysics::High Energy Astrophysical Phenomenaaccretion accretion disks hydrodynamics shock waves stars: pre-main sequence X-rays: starsFOS: Physical sciencesAstronomy and AstrophysicsObservableAstrophysics::Cosmology and Extragalactic AstrophysicsPlasmaAstrophysicsThermal conductionAccretion (astrophysics)T Tauri starSettore FIS/05 - Astronomia E AstrofisicaAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceThermalAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaChromosphereSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsAstronomy & Astrophysics
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ROLE OF EJECTA CLUMPING AND BACK-REACTION OF ACCELERATED COSMIC RAYS IN THE EVOLUTION OF TYPE Ia SUPERNOVA REMNANTS

2012

We investigate the role played by initial clumping of ejecta and by efficient acceleration of cosmic rays (CRs) in determining the density structure of the post-shock region of a Type Ia supernova remnant (SNR) through detailed 3D MHD modeling. Our model describes the expansion of a SNR through a magnetized interstellar medium (ISM), including the initial clumping of ejecta and the effects on shock dynamics due to back-reaction of accelerated CRs. The model predictions are compared to the observations of SN 1006. We found that the back-reaction of accelerated CRs alone cannot reproduce the observed separation between the forward shock (FS) and the contact discontinuity (CD) unless the energ…

High Energy Astrophysical Phenomena (astro-ph.HE)Shock wavePhysicsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and AstrophysicsCosmic rayAstrophysicsShock (mechanics)cosmic rays instabilities ISM: supernova remnants magnetohydrodynamics: MHD shock waves supernovae: individual: SN 1006Interstellar mediumSupernovaSpace and Planetary ScienceAstrophysics::Solar and Stellar AstrophysicsMagnetohydrodynamicsAstrophysics - High Energy Astrophysical PhenomenaEjectaSupernova remnantAstrophysics::Galaxy AstrophysicsThe Astrophysical Journal
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HSP10,HSP70 AND HSP90 IMMUNOHISTOCHEMICAL LEVELS CHANGE IN ULCERATIVE COLITIS AFTER THERAPY

2011

Ulcerative colitis (UC) is a form of inflammatory bowel disease (IBD) characterized by damage of large bowel mucosa and frequent extra-intestinal autoimmune comorbidities. The role played in IBD pathogenesis by molecular chaperones known to interact with components of the immune system involved in inflammation is unclear. We previously demonstrated that mucosal Hsp60 decreases in UC patients treated with conventional therapies (mesalazine, probiotics), suggesting that this chaperonin could be a reliable biomarker useful for monitoring response to treatment, and that it might play a role in pathogenesis. In the present work we investigated three other heat shock protein/molecular chaperones:…

HistologyBiophysicsDown-RegulationInflammationcomorbidity.Inflammatory bowel diseaseulcerative colitis heat shock proteins Hsp molecular chaperones inflammation comorbidity.Pathogenesischemistry.chemical_compoundMesalazineulcerative colitis heat shock proteins Hsp molecular chaperones inflammation comorbidityHeat shock proteinChaperonin 10MedicineHspHumansHSP70 Heat-Shock ProteinsHSP90 Heat-Shock ProteinsColitisMesalaminelcsh:QH301-705.5ulcerative colitisbusiness.industryBrief Reportmolecular chaperonesAnti-Inflammatory Agents Non-SteroidalCell Biologymedicine.diseaseUlcerative colitisImmunohistochemistrydigestive system diseaseschemistrylcsh:Biology (General)inflammationImmunologyheat shock proteinsBiomarker (medicine)Colitis Ulcerativemedicine.symptombusiness
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Cellular responses and HSP70 expression during wound healing in Holothuria tubulosa (Gmelin, 1788).

2014

Wound repair is a key event in the regeneration mechanisms of echinoderms. We studied, at the behavioural, cellular and molecular levels, the wound healing processes in Holothuria tubulosa after injuries to the body wall. The experiments were performed for periods of up to 72 h, and various coelomocyte counts, as well as the expression of heat shock proteins (HS27, HSP70 and HSP90), were recorded. Dermal wound healing was nearly complete within 72 h. In the early stages, we observed the injured animals twisting their bodies to keep their injuries on the surface of the water for the extrusion of the buccal pedicles. At the cellular level, we found time-dependent variations in the circulating…

HolothurianStreImmunoblottingSettore BIO/05 - ZoologiaHSP27 Heat-Shock ProteinsAquatic ScienceAndrologyWestern blotHeat shock proteinmedicineHSPEnvironmental ChemistryAnimalsHolothuriaHSP70 Heat-Shock ProteinsHSP90 Heat-Shock ProteinsSettore BIO/06 - Anatomia Comparata E CitologiaCoelomocyteWound Healingmedicine.diagnostic_testbiologyRegeneration (biology)Holothuria tubulosaGeneral Medicinebiology.organism_classificationHsp70Organ SpecificityImmunologyCoelomocyteWound healingHolothuriaFishshellfish immunology
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