Search results for "Density gradient"

showing 5 items of 55 documents

Description of an improved method for Blastocystis hominis culture and axenization

1996

An improved method for Blastocystis hominis culture and axenization was developed in the present study. Stool samples were cultured in prereduced Boeck-Drbohlav NHI modified medium (with several modifications) supplemented with antibiotics (0.4% ampicillin, 0.1% streptomycin, 0.0006% amphotericin B). Axenization was performed by the combination of partial purification of B. hominis by Ficoll-metrizoic acid gradient and inoculation in fresh medium containing active antibiotics against remaining bacteria. A total of 25 strains were obtained by this procedure. The time required for axenization ranged between 3 and 5 weeks. The generation time of axenic strains ranged from 6.6 to 12.1 h (mean +…

medicine.drug_classAntibioticsBlastocystis InfectionsMicrobiologyFecesAmpicillinAmphotericin BCentrifugation Density GradientmedicineAnimalsHumansBlastocystis hominisAxenicFecesBlastocystisGeneral VeterinarybiologyGeneral Medicinebiology.organism_classificationCulture MediaInfectious DiseasesStreptomycinInsect ScienceParasitologyCell DivisionBacteriamedicine.drugParasitology Research
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Effects on lipoprotein subclasses of combined expression of human hepatic lipase and human apoB in transgenic rabbits

2003

Objective— The effects of combined expression of human hepatic lipase (HL) and human apolipoprotein B (apoB) on low-density lipoprotein (LDL) subclasses were examined in rabbits, a species naturally deficient in HL activity. Methods and Results— In apoB-transgenic rabbit plasma, >80% of the protein was found in the 1.006- to 1.050-g/mL fraction. Gradient gel electrophoresis (GGE) of this fraction revealed two distinct species, designated large and small LDL. A denser fraction (d=1.050 to 1.063 g/mL) contained small LDL as well as another discrete LDL subspecies, designated very small LDL. Expression of HL resulted in reductions in protein concentrations in the 1.006- to 1.050-g/mL densi…

medicine.medical_specialtyApolipoprotein BRecombinant Fusion ProteinsTriacylglycerol lipaseAnimals Genetically ModifiedSpecies SpecificityInternal medicineCentrifugation Density GradientmedicineAnimalsHumansTriglyceridesApolipoproteins BGel electrophoresischemistry.chemical_classificationLagomorphabiologyLipasebiology.organism_classificationAnimal FeedSpecific Pathogen-Free OrganismsLipoproteins LDLMolecular WeightEndocrinologyEnzymechemistrybiology.proteinElectrophoresis Polyacrylamide GelFemalelipids (amino acids peptides and proteins)Density gradient ultracentrifugationRabbitsHepatic lipaseCardiology and Cardiovascular MedicineLipoprotein
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3H-cyproterone acetate: binding characteristics to human uterine progestagen receptors

1985

The availability of tritium labeled cyproterone acetate (CPA) facilitated the systematic investigation of the binding characteristics of this compound for human uterine progesterone receptors (PgR). The binding parameters of 3H-CPA are compared to those of 3H-R5020 and 3H-progesterone. The rate constants of association (k1M-1sec-1) to PgR were 7.8 X 10(3) for 3H-R5020, 4.5 X 10(4) for 3H-progesterone and 4.0 X 10(4) for 3H-CPA. The rate constants of dissociation (k-1, sec-1) were 3.6 X 10(-5) for 3H-R5020, 21.3 X 10(-5) for 3H-progesterone and 17.8 X 10(-5) for 3H-CPA. The Kd-values (M), as obtained by titration analysis and subsequent Scatchard plot analysis were 1.2 X 10(-9) for 3H-R5020,…

medicine.medical_specialtyEndocrinology Diabetes and Metabolismmedicine.medical_treatmentStatistics as TopicTritiumBinding CompetitivePromegestoneSteroidchemistry.chemical_compoundEndocrinologyInternal medicineCentrifugation Density GradientmedicineHumansPotencyheterocyclic compoundsCyproteroneBinding siteCyproterone AcetateReceptorProgesteroneUterusCyproterone acetateKineticsEndocrinologychemistryDihydrotestosteronecardiovascular systemCyproteroneFemaleTritiumReceptors Progesteronehormones hormone substitutes and hormone antagonistsmedicine.drugJournal of Endocrinological Investigation
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In vivo metabolism of LDL subfractions in patients with heterozygous FH on statin therapy

2004

LDL can be subfractionated into buoyant (1.020-1.029 g/ml(-1)), intermediate (1.030-1.040 g/ml(-1)), and dense (1.041-1.066 g/ml(-1)) LDLs. We studied the rebound of these LDL-subfractions after LDL apheresis in seven patients with heterozygous familial hypercholesterolemia (FH) regularly treated by apheresis (58 +/- 9 years, LDL-cholesterol = 342 +/- 87 mg/dl(-1), triglycerides = 109 +/- 39 mg/dl(-1)) and high-dose statins. Apolipoprotein B (apoB) concentrations were measured in LDL subfractions immediately after and on days 1, 2, 3, 5, and 7 after apheresis. Compartmental models were developed to test three hypotheses: 1) that dense LDLs are derived from the delipidation of buoyant and in…

medicine.medical_specialtyVery low-density lipoproteinApolipoprotein Blow density lipoprotein metabolismFamilial hypercholesterolemiaQD415-436Biochemistrychemistry.chemical_compoundEndocrinologyInternal medicinerebound kineticsmedicinesmall dense low density lipoproteinsdensity gradient ultracentrifugationbiologyfamilial hypercholesterolemiaChemistryCholesterollow density lipoprotein subtypesCell BiologyMetabolismmedicine.diseaseEndocrinologyApheresisLDL apheresisbiology.proteinDensity gradient ultracentrifugationlipids (amino acids peptides and proteins)Journal of Lipid Research
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Investigating the Structure of Vela X

2018

Vela X is the prototypical example of a pulsar wind nebula whose morphology and detailed structure have been affected by the interaction with the reverse shock of its host supernova remnant. The resulting complex of filamentary structure and mixed-in ejecta embedded in a nebula that is offset from the pulsar provides the best example we have of this middle-age state that characterizes a significant fraction of composite SNRs, and perhaps all of the large-diameter PWNe seen as TeV sources. Here we report on an XMM-Newton Large Project study of Vela X, supplemented by additional Chandra observations. Through broad spectral modeling as well as detailed spectral investigations of discrete emiss…

shock waveDensity gradientAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsVela01 natural sciencesPulsar wind nebulaPulsar0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010306 general physicsEjectaSupernova remnant010303 astronomy & astrophysicsacceleration of particleISM: supernova remnantAstrophysics::Galaxy AstrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)NebulaAstronomy and AstrophysicsAstronomy and AstrophysicISM: individual objects (Vela X)Space and Planetary ScienceAstrophysics - High Energy Astrophysical PhenomenaEquivalent width
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