363 research outputs found

    Residues of pesticides in soil and water

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    V lončnih poskusih na prostem, brez vegetacije smo zasledovali razkroj in kopičenje prometrina (herbicid - iz skupine triazinov) v dveh različnih talnih tipih, v rendzini in v rjavih tleh. Razkroj prometrina v gornjem sloju rendzine (do 5 cm) s pH = 7 in s povprečno 9-% humusa je potekal v poletnih mesecih štirikrat počasneje, kot na rjavih tleh s pH = 5 do 6 in z manjšo količino humusa – 6%. Bolj enakomerno je potekala migracija v spodnje plasti (do 15 cm). Obratno pa je bila po nadaljnjih 6 mesecih relativna razgradnja prometrina v rjavih tleh v gornjem sloju počasnejša. Za orientacijo o prisotnosti .kloriranih ostankov pesticidov v vodah smo porabili vzorce rib. Znana je, da se v nekaterih delih vodnih živali reziduji pesticidov posebno nakopičijo. Pri analizah vzorcev rib ulovljenih ob slovenski obali Jadranskega morja smo ugotovili prisotnost DDT-ja in njegovih metabolitov. Ponekad je bil v merljivih količinah tuđi dieldrin.In pot experiments in the open, without vegetation, the degradation and accumulation of prometrine (herbicide of the triazine group) in two different soil types, the rendzina and brown soil, were observed. Degradation of prometrine in the upper layer of rendzina (up to 5 cm) with pH = 7 and an average of 9-% humus was in the summer season by 4 times slower than on brown soil with pH = 5-6 and a lesser amount of humus (6%). More regular was migration to the lower layers (up to 15 cm). After six months, however, the relative degradation of prometrine in brown soil was in the upper layer slower. The presence of chlorinated pesticide residues in water was determined or fish samples, since these residues are especially accumulated in some parts of aquatic animals. By analyses of fish samples from the Slovenian coast of the Adriatic, the presence of DDT and its metabolites was established. In some instances also measurable quantities of dieldrin were found

    A Small-Molecule Inhibitor of Mps1 Blocks the Spindle-Checkpoint Response to a Lack of Tension on Mitotic Chromosomes

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    SummaryThe spindle checkpoint prevents chromosome loss by preventing chromosome segregation in cells with improperly attached chromosomes [1–3]. The checkpoint senses defects in the attachment of chromosomes to the mitotic spindle [4] and the tension exerted on chromosomes by spindle forces in mitosis [5–7]. Because many cancers have defects in chromosome segregation, this checkpoint may be required for survival of tumor cells and may be a target for chemotherapy. We performed a phenotype-based chemical-genetic screen in budding yeast and identified an inhibitor of the spindle checkpoint, called cincreasin. We used a genome-wide collection of yeast gene-deletion strains and traditional genetic and biochemical analysis to show that the target of cincreasin is Mps1, a protein kinase required for checkpoint function [8]. Despite the requirement for Mps1 for sensing both the lack of microtubule attachment and tension at kinetochores, we find concentrations of cincreasin that selectively inhibit the tension-sensitive branch of the spindle checkpoint. At these concentrations, cincreasin causes lethal chromosome missegregation in mutants that display chromosomal instability. Our results demonstrate that Mps1 can be exploited as a target and that inhibiting the tension-sensitive branch of the spindle checkpoint may be a way of selectively killing cancer cells that display chromosomal instability

    Radiation pressure instability driven variability in the accreting black holes

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    The time dependent evolution of the accretion disk around black hole is computed. The classical description of the α\alpha-viscosity is adopted so the evolution is driven by the instability operating in the innermost radiation-pressure dominated part of the accretion disk. We assume that the optically thick disk always extends down to the marginally stable orbit so it is never evacuated completely. We include the effect of the advection, coronal dissipation and vertical outflow. We show that the presence of the corona and/or the outflow reduce the amplitude of the outburst. If only about half of the energy is dissipated in the disk (with the other half dissipated in the corona and carried away by the outflow) the outburst amplitude and duration are consistent with observations of the microquasar GRS 1915+105. Viscous evolution explains in a natural way the lack of direct transitions from the state C to the state B in color-color diagram of this source. Further reduction of the fraction of energy dissipated in the optically thick disk switches off the outbursts which may explain why they are not seen in all high accretion rate sources being in the Very High State.Comment: 31 pages, 14 figures; accepted to Ap

    Radiation pressure instability as a variability mechanism in the microquasar GRS 1915+105

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    Physical mechanism responsible for high viscosity in accretion disks is still under debate. Parameterization of the viscous stress as αP\alpha P proved to be a successful representation of this mechanism in the outer parts of the disk, explaining the dwarf novae and X-ray novae outbursts as due to ionization instability. We show that this parameterization can be also adopted in the innermost part of the disk where the adoption of the α\alpha-viscosity law implies the presence of the instability in the radiation pressure dominated region. We study the time evolution of such disks. We show that the time-dependent behavior of GRS 1915+105 can be well reproduced if α\alpha-viscosity disk model is calculated accurately (with proper numerical coefficients in vertically averaged equations and with advection included), and if the model is supplemented with (i) moderate corona dissipating 50% of energy (ii) jet carrying luminosity-dependent fraction of energy. These necessary modifications in the form of the presence of a corona and a jet are well justified observationally. The model predicts outbursts at luminosity larger than 0.16M˙Edd\dot M_{Edd}, as required, correct outburst timescales and amplitudes, including the effect of increasing outburst timescale with mean luminosity. This result strongly suggests that the α\alpha-viscosity law is a good description of the actual mechanism responsible for angular momentum transfer also in the innermost, radiation pressure dominated part of the disk around a black hole.Comment: 6 pages, 2 figures; accepted for publication in ApJ Letter

    Kondo-like transport and magnetic field effect of charge carrier fluctuations in granular aluminum oxide thin films

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    Granular aluminum oxide is an attractive material for superconducting quantum electronics. However, its low-temperature normal state transport properties are still not fully understood, while they could be related to the unconventional phenomenon of the superconductivity in this material. In order to obtain useful information on this aspect, a detailed study of charge carrier fluctuations has been performed in granular aluminum oxide films. The results of electric noise measurements indicate the presence of a Kondo-type spin-flip scattering mechanism for the conducting electrons in the normal state, at low temperatures. Moreover, the magnetic field dependence of the noise amplitude suggests that interface magnetic moments are the main source of fluctuations. The identification of the nature of fluctuation processes is a mandatory requirement for the improvement of quality and performance of quantum devices

    Kondo-like transport and magnetic field effect of charge carrier fluctuations in granular aluminum oxide thin films

    Get PDF
    Granular aluminum oxide is an attractive material for superconducting quantum electronics. However, its low-temperature normal state transport properties are still not fully understood, while they could be related to the unconventional phenomenon of the superconductivity in this material. In order to obtain useful information on this aspect, a detailed study of charge carrier fluctuations has been performed in granular aluminum oxide films. The results of electric noise measurements indicate the presence of a Kondo-type spin-flip scattering mechanism for the conducting electrons in the normal state, at low temperatures. Moreover, the magnetic field dependence of the noise amplitude suggests that interface magnetic moments are the main source of fluctuations. The identification of the nature of fluctuation processes is a mandatory requirement for the improvement of quality and performance of quantum devices
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