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Como descobrir um numero restrito no celular La pgina informativa 17a en www. Como faço para descobrir numero restrito vivo Pero secretamente permanece encendido; Est activo el micrófono y la grabación con la cmara. Como descobrir numero que ligou restrito Realizar compras en su nombre. This variation may be caused by the activity of dark spot on the primary component.

Combining four newly determined times of the light minimum with others published in the literature, the orbital period change of the system was investigated. The period oscillation can be explained either by the light-time effect via the presence of an unseen third body or by magnetic-activity cycles of the components. This indicates that it is on the TRO-controlled stage of the evolutionary scheme proposed by Qian.

The asymmetry of the light curves requires a large, single star spot on the smaller, less massive secondary component.

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The modeled spot varied little during the year range of photometric observations. Among the 16 shallow-contact systems with a decreasing orbital period, MR Com has the lowest mass ratio e. The shallow-contact configuration, the low-mass ratio, and the long-term period decrease all suggest that systems similar to MR Com are on the AML-controlled stage of the evolutionary scheme proposed by Qian. They will oscillate around a critical mass ratio and evolve into a deep contact with a higher mass ratio.

The small-amplitude cyclic change in the O - C curve was analyzed for the light-travel time effect via the presence of an extremely cool stellar companion. The variations of the orbital period were analyzed based on 12 new determined times of light minimum together with the others compiled from the literature. Photometric solutions determined with the Wilson-Devinney method suggest that BI CVn is a contact binary with a degree of contact of The asymmetry of the light curves was interpreted by the presence of dark spots on both components, and absolute parameters were determined by combining the photometric elements with the spectroscopic solutions given by Lu.

The observed period decrease can be plausibly explained by a combination of the mass transfer from the primary to the secondary and angular momentum loss via magnetic braking. The cyclic period oscillation suggests that BI CVn is a triple system containing a tertiary component with a mass no less than 0. As in the cases of the other contact binaries e. The classical explosive basaltic eruption spectrum is traditionally defined by the following end member eruption styles: The field use of high-speed cameras has enabled volcanologists to make improved quantifications and more accurate descriptions of these classical eruptions styles and to quantify previously undecipherable activity including activity on the basaltic eruption spectrum between the two defined end members.

Explosive activity in at the free surface of the Halema' uma 'u lava lake at Kilauea exhibited features of both sustained Hawaiian fountaining and transient Strombolian explosivity. Most of this activity is internally triggered by the internal rise of decoupled gas bubbles from below the lake's surface, but external triggering via rock falls, was also observed.

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Here I identify three styles of bubble bursting and spattering eruptive activity isolated events, clusters of events, and prolonged episodes at the lava lake, and distinguished them based on their temporal and spatial distributions. Isolated events are discrete single bubble bursts that persist for a few tenths of seconds to seconds and are separated by repose periods of similar or longer time scales.

Cluster of events are closely spaced, repeated events grouped around a narrow point source, which persist for seconds to minutes. Prolonged episodes are groupings of numerous events closely linked in space and time that persist for tens of minutes to hours. Analysis of individual events from high-speed camera images indicates that they are made up of up to three phases: Based on the numerical parameters established in this study, the activity was relatively weak i.

We present a detailed analysis of the interesting W UMa binary FI Boo in view of the spectroscopic signature of a third body through photometry, period variation, and a thorough investigation of solution uniqueness. The results were tested by heuristic scanning and parameter kicking to provide the consistent and reliable set of parameters that was used to obtain the initial masses of the progenitors 1.

We also investigated the evolutionary status of massive components with several sets of widely used isochrones. However, it has been neglected in photometric investigations. Here, the first complete light curves in the B, V, R, and I bands are presented and analyzed using the Wilson and Devinney method. The continuous increase may be caused by a mass transfer from the less massive component to the more massive one. This suggests that UZ CMi is in the thermal relaxation oscillation controlled stage of the evolutionary scheme proposed by Qian.

UZ CMi will oscillate around a critical mass ratio and the contact configuration cannot be broken. The cyclic change was analyzed for the light-travel time effect via the presence of an extremely cool stellar companion. The formation, evolution, collapse, and subsequent resurrection of a vent within Halema' uma 'u Crater, Kilauea Volcano, produced energetic and varied degassing signals recorded by a nearby infrasound array between and early After 25 years of quiescence, a vent-clearing explosive burst on 19 March produced a clear, complex acoustic signal.

Near-continuous harmonic infrasonic tremor followed this burst until 4 December , when a period of decreased degassing occurred. The tremor spectra suggest volume oscillation and reverberation of a shallow gas-filled cavity beneath the vent. The dominant tremor peak can be sustained through Helmholtz oscillations of the cavity, while the secondary tremor peak and overtones are interpreted assuming acoustic resonance. The dominant tremor frequency matches the oscillation frequency of the gas emanating from the vent observed by video.

Over 21 varied degassing bursts were observed with extended burst durations and frequency content consistent with a transient release of gas exciting the cavity into resonance. Correlation of infrasound with seismicity suggests an open system connecting the atmosphere to the seismic excitation process at depth. Numerous degassing bursts produced very long period 0. Kilauea infrasound appears controlled by the exsolution of gas from the magma, and the interaction of this gas with the conduits and cavities confining it. Using the lava lake as the hot background source we present MWIR gas analysis of the Kilauea volcanic plume.

A total of 76 times of light minima were collected and listed in Table 2. The minimum scatter, 0. The light travel effect produced by the presence of tertiary components can reveal much about the origin and evolution of over-contact binaries. Progress in the analysis of eclipse timing variations is summarized here both from the empirical and the theoretical points of view, and a more extensive investigation of the proposed orbital parameters of third bodies is proposed.

The code we have developed for this, implemented in Python, is set up to handle heuristic scanning with parameter perturbation in parameter space, and to establish realistic uncertainties from the least squares fitting.

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Future options to be implemented include MCMC and bootstrapping. We present the first precision BVRI light curves, synthetic light curve solutions, and a period study for the high amplitude solar type binary, V Cygni. The light curves have the appearance of an Algol EA type; however, it is made up of dwarf solar type components in a detached mode with a period of only 0. Flare-like disruptions occur in the light curves following the primary and secondary eclipses possibly due to the line-of-sight track of a gas stream.

The more massive star is the gainer, making this system a classic, albeit dwarf, Algol. Survey of period variations of superhumps in SU UMa -type dwarf novae. The eighth year Continuing the project described by Kato et al. The data have improved the distribution of orbital periods, the relation between the orbital period and the variation of superhumps, and the relation between period variations and the rebrightening type in WZ Sge-type objects.

Coupled with new measurements of mass ratios using growing stages of superhumps, we now have a clearer and statistically greatly improved evolutionary path near the terminal stage of evolution of cataclysmic variables. We have newly obtained superhump periods for 79 objects and 13 orbital periods, including periods from early superhumps.

In order that future observations will be more astrophysically beneficial and rewarding to observers, we propose guidelines on how to organize observations of various superoutbursts. The measurements were obtained using inch and 1-inch telescopes, respectively. The observations were performed at the Masaryk University Observatory in Brno 3 nights, inch , and at the private observatory in Brno 16 nights, 1-inch in the Czech Republic from December to June Exposures were v - 60s, b - 30s, y - 30s, green - 30s.

For the small aperture telescope, five frames were combined to a single image to achieve a better signal-to-noise ratio. The time resolution of a such combined frame is about s. CCD images were calibrated in a standard way dark frame and flat field corrections. The C-Munipack software Motl was used for this processing as well as for differential photometry.

The 4th file contains minima timings of eclipsing binary CL Aur. In , the National Educational Reform in Bolivia instituted reforms that called for a model of education that held at its center the knowledge and languages of Indigenous people. The types of change called for by the reforms in Bolivia signify major transformations in teacher preparation practices and a concerted emphasis on training in….

Documento de Politica Sectorial. The present paper updates the World Bank's interpretations of education development and outlines a policy framework for lending for education. After chapters on the relationship between education and development and on the state of education development, the paper devotes a chapter to each of five issues: A Political, Economic, and Social View. This address seeks to explain in brief the historical background and political, economic, and social conditions leading to the democratic election of a Marxist president in Chile.

A historical sketch of Chilean government from independence in is provided with a description of the situation just before Salvador Allende's election in Politicas de uniformes y codigos de vestuario Uniforms and Dress-Code Policies. This digest in Spanish examines schools' dress-code policies and discusses the legal considerations and research findings about the effects of such changes. Most revisions to dress codes involve the use of uniforms, typically as a way to curb school violence and create a positive learning environment.

A recent survey of secondary school principals…. El medio ambiente de las politicas Standards: This digest in Spanish offers a snapshot of the standards movement: While a broad coalition of constituencies has embraced standards-based reform as a means of improving…. A revised ephemeris and updated orbital period for EQ Tau have been determined from newly acquired CCD-derived photometric data. A Roche-type model based on the Wilson-Devinney code produced simultaneous theoretical fits of light curve data in three passbands by invoking cold spots on the primary component.

These new model fits, along with similar light curve data for EQ Tau collected during the previous six seasons , provided a rare opportunity to follow the seasonal appearance of star spots on a W UMa binary system over nine consecutive years. Fixed values for q,?

With the exception of the season all other light curves produced since then required a spotted solution to address the flux asymmetry exhibited by this binary system at Max I and Max II. At least one cold spot on the primary appears in seven out of twelve light curves for EQ Tau produced over the last nine years, whereas in six instances two cold spots on the primary star were invoked to improve the model fit. Solutions using a hot spot were less common and involved positioning a single spot on the primary constituent during the , , and seasons. In many industrial areas such as in food, pharmaceutical, cosmetic, printing, and textile, the use of synthetic dyes has been integral with products such as azo dye, anthrax, and dyestuffs.

As such, these industries produce a lot of waste by-products that could contaminate the environment. Bioremediation, therefore, has become an important emerging technology due to its cost-sustainable, effective, natural approach to cleaning up contaminated groundwater and soil via the use of microorganisms. The use of microorganisms in bioremediation requires the optimisation of parameters used in cultivating the organism. Biodegradation analyses were carried out on a soil spiked with RBBR and supplemented with rice husk as the fungus growth enhancer.

A two-level Plackett-Burman design was used to screen the medium components for the effects on the decolourization of RBBR. To describe the clinical course of paediatric patients undergoing surgery for congenital heart disease in UMAE of Yucatan.

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Descriptive review was performed on the records of paediatric patients undergoing surgery for congenital heart disease from 1 November to 30 November The most frequent heart diseases were persistent ductus arteriosus The median intensive care stay was 3 days. The most frequent complications were sepsis 5.

There was a moderate positive correlation between surgical complications and survival or death. The number of surgical patients is lower compared to reference centres for cardiovascular surgery. There is a marked tendency to perform corrective and palliative surgeries in specific disease in patients with added risk or 'bad' cardiac anatomy that prevent full correction at the first attempt.

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Prospective epidemiological and clinical studies should be conducted to understand the behaviour of congenital heart diseases treated in the region. The orbital period decrease was found to be a rate of The inner and outer critical Roche lobes will contract and cause the contact degree to increase.

Therefore, IK Boo may evolve into a deeper contact system. Furthermore, a possible cyclic variation was found with a period of 9.

Speciation, population structure, and demographic history of the Mojave Fringe-toed Lizard Uma scoparia , a species of conservation concern. The North American deserts were impacted by both Neogene plate tectonics and Quaternary climatic fluctuations, yet it remains unclear how these events influenced speciation in this region. We tested published hypotheses regarding the timing and mode of speciation, population structure, and demographic history of the Mojave Fringe-toed Lizard Uma scoparia , a sand dune specialist endemic to the Mojave Desert of California and Arizona.

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We sampled individual lizards representing 22 insular dune localities, obtained DNA sequences for 14 nuclear loci, and found that U. Analyses of genotypes using Bayesian clustering algorithms did not identify discrete populations within U. Using isolation-with-migration IM models and a novel coalescent-based hypothesis testing approach, we estimated that U. The likelihood ratio test and the Akaike Information Criterion consistently rejected nested speciation models that included parameters for migration and population growth of U.

We reject the Neogene vicariance hypothesis for the speciation of U. It is a high-amplitude V 0. As expected, the light curve is asymmetric due to spot activity. Three times of minimum light were calculated, for two primary eclipses and one secondary eclipse, from our present observations. In total, some 26 times of minimum light covering nearly 20 years of observation were used to determine linear and quadratic ephemerides. It is noted that the light curve solution remained in a detached state for every iteration of the computer runs.

A degree radius high latitude white spot faculae was iterated on the primary component. Three new precise epochs of minimum light were determined and a linear and a quadratic ephemeris were computed from these and previous data covering 28 years of observation. The light curves reveal that the system undergoes a brief 20 min totality in the primary eclipse, indicating that CE Leo is a W UMa W-type binary.

Standard magnitudes were found and a simultaneous solution of the B, V, R, I light curves was computed using the new Wilson-Devinney synthetic light curve code which has the capability of automatically adjusting star spots.

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Mas poucas sabem disso. New photometric observations of a W UMa system, V Aur, were carried out over 10 nights from December 19 to February 8, from which four sets of light curves were obtained. The C-Munipack software Motl was used for this processing as well as for differential photometry. Monitorear multiples dispositivos Al mismo tiempo puede monitorear smartphones Android, iOS y computadoras Mac, Windows. Recent category: Como se puede acceder al whatsapp de otra persona espiar otro celular desde mi pc rastrear telefono por imei android como espiar un telefono sin instalar nada. The components of the partially-eclipsed MM Peg have close parameters. They usually have EA or EB-type light curves unequal eclipse depths, indicating components with substantially different temperatures.

The solution indicates that the system consists of two early K-type dwarfs in marginal contact with a fill-out factor less than 3 percent. Evidence for the presence of a large 45 deg radius superluminous area on the cooler component is given. Environmental differences in substrate mechanics do not affect sprinting performance in sand lizards Uma scoparia and Callisaurus draconoides. Running performance depends on a mechanical interaction between the feet of an animal and the substrate. This interaction may differ between two species of sand lizard from the Mojave Desert that have different locomotor morphologies and habitat distributions.

Uma scorparia possesses toe fringes and inhabits dunes, whereas the closely related Callisaurus draconoides lacks fringes and is found on dune and wash habitats. The present study evaluated whether these distribution patterns are related to differential locomotor performance on the fine sand of the dunes and the course sand of the wash habitat. We measured the kinematics of sprinting and characterized differences in grain size distribution and surface strength of the soil in both habitats.

Although wash sand had a surface strength The broadly distributed C. Furthermore, there were no significant differences in maximum acceleration or the time to attain maximum speed between species or between substrates. These results suggest that differences in habitat distribution between these species are not related to locomotor performance and that sprinting ability is dominated neither by environmental differences in substrate nor the presence of toe fringes.

Size-resolved chemistry of aerosols produced by Halema' uma 'u eruption , Kilauea Volcano, Hawai'i. A dense quiescent plume has been emitted continuously from the eruptive vent in Halema' uma 'u crater since March Aerosol particles were sampled near-source in the young plume uma 'u and Pu'u O'o show SO in the same narrow size bin 0.

It is noteworthy that the particles appear not to have grown when the plume has drifted km downwind. The formation of aerosol measured downwind is dominated by oxidation of SO2 to SO in the plume. Um total de 5. These solar-type systems are usually detached or semidetached with one or both components under filling their critical Roche lobes.

They usually have EA or EB-type light curves unequal eclipse depths, indicating components with substantially different temperatures. The accepted scenario for these W UMa binaries is that they are undergoing steady but slow angular momentum losses due to magnetic braking as stellar winds blow radially away on stiff bipolar field lines. These binaries are believed to come into stable contact and eventually coalesce into blue straggler type, single, fast rotating A-type stars Guinan and Bradstreet, This is the shortest period PCWB found so far.

Our solutions of light curves separated by some three years give approximately the same physical parameters. However the spots radically change, in temperature, area and position causing a distinctive variation in the shape of the light curves. We conclude that spots are very active on this solar type dwarf system and that it may mimic its larger cousins, the RS CVn binaries.

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