J/A+A/634/A9    PKS 1549-79 ALMA data cubes & continuum images (Maccagni+, 2020)

The flickering nuclear activity of Fornax A. Maccagni F.M., Murgia M., Serra P., Govoni F., Morokuma-Matsui K., Kleiner D., Buchner S., Jozsa G.I.G., Kamphuis P., Makhathini S., Molnar D.Cs., Prokhorov D.A., Ramaila A., Ramatsoku M., Thorat K., Smirnov O. <Astron. Astrophys. 634, A9 (2020)> =2020A&A...634A...9M 2020A&A...634A...9M (SIMBAD/NED BibCode)
ADC_Keywords: Galaxies, radio ; Radio sources Keywords: galaxies: individual: Fornax A - galaxies: individual: NGC 1316 - galaxies: active - radio continuum: galaxies - galaxies: jets - radiation mechanisms: non-thermal Abstract: We present new observations of Fornax A taken at ∼1GHz with the MeerKAT telescope and at ∼6GHz with the Sardinia Radio Telescope (SRT). The sensitive (noise ∼16uJy/beam), high-resolution (<10'') MeerKAT images show that the lobes of Fornax A have a double-shell morphology, where dense filaments are embedded in a diffuse and extended cocoon. We study the spectral properties of these components by combining the MeerKAT and SRT observations with archival data between 84MHz and 217GHz. For the first time, we show that multiple episodes of nuclear activity must have formed the extended radio lobes. The modelling of the radio spectrum suggests that the last episode of injection of relativistic particles into the lobes started ∼24Myr ago and stopped 12Myr ago. More recently (∼3Myr ago), a less powerful and short (<1Myr) phase of nuclear activity generated the central jets. Currently, the core may be in a new active phase. It appears that Fornax A is rapidly flickering. The dense environment around Fornax A has lead to a complex recent merger history for this galaxy, including mergers spanning a range of gas contents and mass ratios, as shown by the analysis of the galaxy's stellar- and cold-gas phases. This complex recent history may be the cause of the rapid, recurrent nuclear activity of Fornax A. Description: 1GHz and 6GHz images of Fornax A taken with the MeerKAT and SRT telescopes. Tables with the flux spectral flux density of different components of Fornax A between 84MHz and 217GHz. Objects: --------------------------------------------- RA (2000) DE Designation(s) --------------------------------------------- 03 22 41.7 -37 12 30 Fornax A = NGC 1316 --------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file tableb1.dat 88 52 Flux densities of Fornax A between 84MHz and 217GHz list.dat 119 9 List of fits images fits/* . 9 Individual fits images -------------------------------------------------------------------------------- Byte-by-byte Description of file:tableb1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 F8.4 GHz Freq Frequency of measured flux density of Fornax A 11- 12 A2 --- n_Freq Note (1) 15- 19 F5.1 Jy FluxDens ? Flux density measured in this work 20 A1 --- u_FluxDens [)] Uncertainty flag on FluxDens 22- 26 F5.1 Jy e_FluxDens ? Error on flux density 28- 34 F7.1 Jy FluxDensMcK ? Flux density measured by McKinley et al. 2015MNRAS.446.3478M 2015MNRAS.446.3478M 37- 38 I2 % e_FluxDensMcK ? Percentage error on flux density 41- 43 I3 Jy FluxDensPer ? Flux density measured by Perley et al. 2017ApJS..230....7P 2017ApJS..230....7P, Cat. J/ApJS/230/7 45- 46 I2 % e_FluxDensPer ? Percentage error on flux density 49- 88 A40 -- Ref Telescope used for the measurements, or the reference to the published fluxes -------------------------------------------------------------------------------- Note (1): Note on Freq as follows: * = indicates flux densities that have not been included in the study of the SED ** = WMAP: Wilkinson Microwave Anisotropy Probe (Bennett et al. 2013ApJS..208...20B 2013ApJS..208...20B, Cat. J/ApJS/208/20) -------------------------------------------------------------------------------- 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- 50 A21 "datime" Obs.date Observation date 52- 56 I5 Kibyte size Size of FITS file 58- 85 A28 --- FileName Name of FITS file, in subdirectory fits 87-119 A33 --- Title Title of the FITS file -------------------------------------------------------------------------------- Acknowledgements: Filippo Maccagni, filippo.maccagni(at)inaf.it
(End) Patricia Vannier [CDS] 23-Jan-2020
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line