74,036 research outputs found

    The Radio and Gamma-Ray Luminosities of Blazars

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    Based on the γ\gamma-ray data of blazars in the third EGRET catalog and radio data at 5 GHz, we studied the correlation between the radio and γ\gamma-ray luminosities using two statistical methods. The first method was the partial correlation analysis method, which indicates that there exist correlations between the radio and γ\gamma-ray luminosities in both high and low states as well as in the average case. The second method involved a comparison of expected γ\gamma-ray luminosity distribution with the observed data using the Kolmogorov-- Smirnov (KS) test. In the second method, we assumed that there is a correlation between the radio and γ\gamma-ray luminosities and that the γ\gamma-ray luminosity function is proportional to the radio luminosity function. The KS test indicates that the expected gamma-ray luminosity distributions are consistent with the observed data in a reasonable parameter range. Finally, we used different γ\gamma-ray luminosity functions to estimate the possible 'observed' γ\gamma-ray luminosity distributions by GLAST.Comment: 8 pages, 4 figures, one table, PASJ, 53 (2001

    Thermal elastohydrodynamic lubrication of spur gears

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    An analysis and computer program called TELSGE were developed to predict the variations of dynamic load, surface temperature, and lubricant film thickness along the contacting path during the engagement of a pair of involute spur gears. The analysis of dynamic load includes the effect of gear inertia, the effect of load sharing of adjacent teeth, and the effect of variable tooth stiffness which are obtained by a finite-element method. Results obtained from TELSGE for the dynamic load distributions along the contacting path for various speeds of a pair of test gears show patterns similar to that observed experimentally. Effects of damping ratio, contact ratio, tip relief, and tooth error on the dynamic load were examined. In addition, two dimensionless charts are included for predicting the maximum equilibrium surface temperature, which can be used to estimate directly the lubricant film thickness based on well established EHD analysis

    Transient effect of lubricant on elastohydro-dynamic film thickness

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    The inlet solution of the elastohydrodynamic lubricated rolling contact problem was obtained by considering lubricants with transient viscosity. The effect of the viscoelastic retardation time of the lubricant on the center film thickness was investigated. The effect of transient viscosity in response to a sudden pressure was found to be insignificant in determining the film thickness in elastohydrodynamic contacts

    Polarization and Variations of BL Lacertae Objects

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    BL Lacertae objects are an extreme subclass of AGNs showing rapid and large-amplitude variability, high and variable polarization, and core-dominated radio emissions. If a strong beaming effect is the cause of the extreme observation properties, one would expect that these properties would be correlated with each other. Based on the relativistic beaming model, relationships between the polarization and the magnitude variation in brightness, as well as the core- dominance parameter are derived and used statistically to compare with the observational data of a BL Lacertae object sample. The statistical results are consistent with these correlations, which suggests that the polarization, the variation, and the core-dominance parameter are possible indications of the beaming effect.Comment: 6 pages, two figures, one table, some revisions. PASJ, 53 (2001

    Colouration in crab spiders: substrate choice and prey attraction

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    Published version: http://jeb.biologists.org/content/208/10/1785/F3.expansio

    Basic properties of Gamma-ray loud blazars

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    In this paper, a method is proposed to determine the basic properties of γ\gamma-ray loud blazars, among them the central black hole mass, M, the Doppler factor, δ\delta, the propagation angle of the γ\gamma-rays with respect to the symmetric axis of a two-temperature accretion disk, Φ\Phi, and the distance (i.e. the height above the accretion disk), d at which the γ\gamma-rays are created, for seven γ\gamma-ray loud blazars with available GeV variability timescales and in which the absorption effect of a γ\gamma-ray and the beaming effect have been taken into account. Our results indicate that, if we take the intrinsic γ\gamma-ray luminosity to be λ\lambda times the Eddington luminosity, Lγin=λLEdd.L_{\gamma}^{in} = \lambda L_{Edd.}, the masses of the blazars are in the range of (4∼131)×107M⊙(4 \sim 131)\times 10^{7}M_{\odot}, the Doppler factors (δ\delta) lie in the range of 0.57 to 5.33 the angle (Φ\Phi) is in the range of 13∘13^{\circ} to 43∘^{\circ} and the distance (d) is in the range of 26R_{g} to 411R_{g}. Our model results are independent of γ\gamma-ray emission mechanisms but they do depend on the X-ray emission mechanism of the accretion disk.Comment: 14 pages, 3 tables, A&A accepte

    The role of UV in crab spider signals: effects on perception by prey and predators

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    Australian crab spiders Thomisus spectabilis sit on the petals of flowers and ambush prey such as honeybees. White-coloured T. spectabilis reflect in the UV (UV+ spiders) and previous research has shown that their presence, curiously, attracts honeybees to daisies. We applied an UV-absorber (Parsol®) to create UV-absorbing (UV–) spiders that did not reflect any light below 395 nm wavelength. These physical changes of visual signals generated by crab spiders caused honeybees to avoid flowers with UV– spiders on their petals. They also affected the perception of UV– spiders by honeybees and a potential avian predator (blue tits). Compared to UV+ spiders, UV– spiders produced less excitation of the UV-photoreceptors in honeybees and blue tits, which translated into a reduced UV-receptor contrast and a reduced overall colour contrast between UV– spiders and daisy petals. Our results reveal that a clean physical elimination of reflection in the UV range affects perception in predators and prey and ultimately changes the behaviour of prey.7 page(s
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