1,088 research outputs found

    86, 43, and 22 GHz VLBI Observations of 3C120

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    We present the first 86 GHz VLBI observations of the radio galaxy 3C~120, together with contemporaneous 43 and 22 GHz polarimetric VLBA observations. The very high angular resolution obtained at 86 GHz provides an upper limit to the size of the core of 54 ÎŒ\muas (0.025 h−1h^{-1}pc). This represents a direct determination of the base of the jet which is independent of variability arguments (which depend on uncertain estimates of the Doppler factor), and places it below approximately one light-month. Comparison with previous VLBA observations after a one-year interval shows pronounced changes in the structure and polarization of the jet. Most of the components are found to follow a curved path while undergoing a steepening of their spectra accompanied by a decrease in total and polarized emission. However, at least one component is observed to follow a quasi-ballistic motion, accompanied by a flattening of its spectrum, as well as an increase in total and polarized flux. This may be explained by its interaction with the external medium, resulting in a shock that enhances the emission and aligns the magnetic field perpendicular to the component motion, thereby producing an increase of the degree of polarization from undetected values to as high as 15%. A second strong component, with the highest degree of polarization (23%), is found to have experienced a displacement from the ridge line of the structural position angle of the jet as it moved downstream. We have found a mean swing to the south of the position angle of the innermost components of ∌6∘\sim 6^{\circ} between late 1996 and 1997, which may be responsible for the jet curvature observed at parsec and kiloparsec scales.Comment: 12 pages, 1 figure. Accepted for publication in ApJ Letter

    Monthly 43 GHz VLBA Polarimetric Monitoring of 3C120 over 16 Epochs: Evidence for Trailing Shocks in a Relativistic Jet

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    We present a 16-month sequence of monthly polarimetric 43 GHz VLBA images of the radio galaxy 3C 120. The images probe the inner regions of the radio jet of this relatively nearby superluminal radio galaxy at a linear resolution of 0.07 h65−1h_{65}^{-1} pc (Ho=65h65H_o= 65 h_{65} km s−1^{-1} Mpc−1^{-1}). We follow the motion of a number of features with apparent velocities between 4.01±\pm0.08 and 5.82±0.13h65−1c5.82\pm 0.13 h_{65}^{-1} c. A new superluminal knot, moving at 4.29±0.16h65−1c4.29\pm 0.16 h_{65}^{-1} c, is observed to be ejected from the core at a time coincident with the largest flare ever observed for this source at millimeter wavelengths. Changes in the position angle of this component, as well as a progressive rotation of its magnetic polarization vector, suggest the presence of a twisted (resembling a helix in projection) configuration of the underlying jet magnetic field and jet geometry. We identify several knots that appear in the wake of the new superluminal component, moving at proper motions ∌4\sim 4 times slower than any of the other moving knots observed in 3C 120. These features have properties similar to those of the ``trailing'' shocks seen in relativistic, time-dependent, hydrodynamical and emission simulations of compact jets. Such trailing compressions are triggered by pinch-mode jet-body instabilities caused by the propagation of a strong perturbation, which we associate with the new strong superluminal component.Comment: 4 pages, 5 figures, accepted for publication in Astrophysical Journal Letter

    El equus stenonis cocchi como indicador biostatigråfico del plio-pleistoceno en Italia y España

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    [Resumen] Se esquematiza la cronoestratigrafía de los principales yacimientos de Vertebrados italianos del Plio-pleistoceno, de el Villafranquiense medio al Galerino. Se estudia, desde un punto de vista evolutivo, la presencia de las distintas formas de Equus stenonis Cocchi hasta la llegada de Equus caballus Linn. La comparación de los distintos estadios evolutivos de E. stenonis y su fauna acompañante permiten la elaboración de un Cuadro sinóptico en el cual los yacimientos españoles con Equus se correlacionan con sus sincrónicos italianos sobre una base estratigråfica comparada (BONADONNA, 1982; ARIAS et all., 1982) con los principales eventos geológicos en Europa[Abstract] The chronostratigraphy of the Plio-pleistocene marnmals italian deposits from middle Villafranchian to Galerian is surnmarized. The presence of different forms of Equus stenonis Cocchi until the appearance of the first kinds of Equus caballus Linn. is studied by an evolutive point of view. The comparison among the different evolutive levels of Equus stenonis and the associated fauna allow us to build a synoptic Table in which the spanish deposits with Equus are correlate to analogous italian ones ln a stratigraphic scale yet compared (BONADONNA, 1982; ARIAS et all., 1982) to the most important geological event ln Europ
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