J/A+A/641/A40     S5 0836+710 Ground and Space VLBI images  (Vega Garcia+, 2020)

Multiband RadioAstron space VLBI imaging of the jet in quasar S5 0836+710. Vega Garcia L., Lobanov A.P., Perucho M., Bruni G., Ros E., Anderson J.M., Agudo I., Davis R., Gomez J.L., Kovalev Y.Y., Krichbaum T.P., Lisakov M., Savolainen T., Schinzel F.K., Zensus J.A. <Astron. Astrophys. 641, A40 (2020)> =2020A&A...641A..40V 2020A&A...641A..40V (SIMBAD/NED BibCode)
ADC_Keywords: QSOs ; Radio sources ; VLBI Keywords: radio continuum: galaxies - galaxies: jets - galaxies: active - galaxies: individual: S5 0836+710 Abstract: Detailed studies of relativistic jets in active galactic nuclei (AGN) require high-fidelity imaging at the highest possible resolution. This can be achieved using very long baseline interferometry (VLBI) at radio frequencies, combining worldwide (global) VLBI arrays of radio telescopes with a space-borne antenna on board a satellite. We present multiwavelength images made of the radio emission in the powerful quasar S5 0836+710, obtained using a global VLBI array and the antenna Spektr-R of the RadioAstron mission of the Russian Space Agency, with the goal of studying the internal structure and physics of the relativistic jet in this object. The RadioAstron observations at wavelengths of 18cm, 6cm, and 1.3cm are part of the Key Science Program for imaging radio emission in strong AGN. The internal structure of the jet is studied by analyzing transverse intensity profiles and modeling the structural patterns developing in the flow. The RadioAstron images reveal a wealth of structural detail in the jet of S5 0836+710 on angular scales ranging from 0.02mas to 200mas. Brightness temperatures in excess of 1013K are measured in the jet, requiring Doppler factors of ≥100 for reconciling them with the inverse Compton limit. Several oscillatory patterns are identified in the ridge line of the jet and can be explained in terms of the Kelvin-Helmholtz (KH) instability. The oscillatory patterns are interpreted as the surface and body wavelengths of the helical mode of the KH instability. The interpretation provides estimates of the jet Mach number and of the ratio of the jet to the ambient density, which are found to be Mj~=12 and η~=0.33. The ratio of the jet to the ambient density should be conservatively considered an upper limit because its estimate relies on approximations. Description: RadioAstron imaging observations of S5 0836+710 were performed at two epochs: on 24 October 2013 at L band (1.6GHz, wavelength λ=18cm) and on 10-11 January 2014 at C band (5GHz, λ=6cm) and K band (22GHz, λ=1.3cm), combining data recorded at the SRT with data provided by a ground array of radio telescopes. At each epoch the source was observed for about 18 hours, starting from a perigee passage of the SRT, in order to ensure a continuous coverage of Fourier domain (uv coverage) by the ground-space baseline data. Ground and space VLBI images. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file list.dat 231 8 List of fits images fits/* . 8 Individual fits images -------------------------------------------------------------------------------- See also: J/A+A/545/A65 : S5 0836+710 image at 1.6GHz (Perucho+, 2012) J/A+A/631/A49 : LOFAR images of blazar S5 0836+710 (Kappes+, 2019) Byte-by-byte Description of file: list.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 F9.5 deg RAdeg Right Ascension of center (J2000) 10- 18 F9.5 deg DEdeg Declination of center (J2000) 20- 23 I4 --- Nx Number of pixels along X-axis 25- 28 I4 --- Ny Number of pixels along Y-axis 30- 39 A10 "date" Obs.date Observation date 41- 48 F8.5 GHz Freq Observed frequency 50- 54 I5 Kibyte size Size of FITS file 56- 82 A27 --- FileName Name of FITS file, in subdirectory fits 84-231 A148 --- Title Title of the FITS file -------------------------------------------------------------------------------- Acknowledgements: Andrei Lobanov, alobanov(at)mpifr-bonn.mpg.de
(End) Patricia Vannier [CDS] 31-Aug-2020
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