4.7 Article

Placing LOFAR-detected quasars in CIV emission space: implications for winds, jets and star formation

期刊

出版社

OXFORD UNIV PRESS
DOI: 10.1093/mnras/stab302

关键词

accretion, accretion discs; galaxies: jets; quasars: emission lines; quasars: general; galaxies: star formation; radio continuum: galaxies

资金

  1. Science and Technology Facilities Council (STFC)
  2. Herchel Smith Fellowship at Cambridge
  3. STFC via the Institute of Astronomy, Cambridge, Consolidated Grant
  4. Royal Society
  5. European Research Council
  6. NOVA
  7. NWO
  8. CNRS-INSU
  9. SURF Co-operative
  10. UK Science and Technology Funding Council
  11. Julich Supercomputing Centre
  12. Alfred P. Sloan Foundation
  13. U.S. Department of Energy Office of Science
  14. Brazilian Participation Group
  15. Carnegie Institution for Science
  16. Carnegie Mellon University
  17. Center for Astrophysics \ Harvard Smithsonian
  18. Chilean Participation Group
  19. French Participation Group
  20. Instituto de Astrofisica de Canarias
  21. The Johns Hopkins University
  22. Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo
  23. Korean Participation Group
  24. Lawrence Berkeley National Laboratory
  25. Leibniz Institut fur Astrophysik Potsdam (AIP)
  26. MaxPlanck-Institut fur Astronomie (MPIA Heidelberg)
  27. Max-PlanckInstitut fur Astrophysik (MPA Garching)
  28. Max-Planck-Institut fur Extraterrestrische Physik (MPE)
  29. National Astronomical Observatories of China
  30. New Mexico State University
  31. New York University
  32. University of Notre Dame
  33. Observatario Nacional/MCTI
  34. The Ohio StateUniversity
  35. Pennsylvania State University
  36. ShanghaiAstronomical Observatory
  37. United Kingdom Participation Group
  38. Universidad Nacional Autonoma de Mexico
  39. University of Arizona
  40. University of Colorado Boulder
  41. University of Oxford
  42. University of Portsmouth
  43. University of Utah
  44. University of Virginia
  45. University of Washington
  46. University of Wisconsin
  47. Vanderbilt University
  48. Yale University
  49. Center for High Performance Computing at the University of Utah

向作者/读者索取更多资源

By investigating the low-frequency radio and ultraviolet properties of a sample of around 10,500 quasars, it was found that the radio detection rate increases with blueshift while the radio-loud fraction decreases. The radio-quiet population shows a range of He II equivalent widths, while the radio-loud population mostly exhibits strong He II. The presence of similar ultraviolet properties but differing radio properties among quasars suggests that radio and ultraviolet emission may be tracing activity occurring on different time-scales.
We present an investigation of the low-frequency radio and ultraviolet properties of a sample of similar or equal to 10 500 quasars from the Sloan Digital Sky Survey Data Release 14, observed as part of the first data release of the Low-Frequency-Array Two-metre Sky Survey. The quasars have redshifts 1.5 < z < 3.5 and luminosities 44.6 < log(10) (L-bol/erg s(-1)) < 47.2. We employ ultraviolet spectral reconstructions based on an independent component analysis to parametrize the CIV.1549-emission line that is used to infer the strength of accretion disc winds, and the He II.1640 line, an indicator of the soft X-ray flux. We find that radio-detected quasars are found in the same region of CIV blueshift versus equivalent-width space as radio-undetected quasars, but that the loudest, most luminous and largest radio sources exist preferentially at low CIV blueshifts. Additionally, the radio-detection fraction increases with blueshift whereas the radio-loud fraction decreases. In the radio-quiet population, we observe a range of He II equivalent widths as well as a Baldwin effect with bolometric luminosity, whilst the radio-loud population has mostly strong He II, consistent with a stronger soft X-ray flux. The presence of strong He II is a necessary but not sufficient condition to detect radio-loud emission suggesting some degree of stochasticity in jet formation. Using energetic arguments and Monte Carlo simulations, we explore the plausibility of winds, compact jets, and star formation as sources of the radio quiet emission, ruling out none. The existence of quasars with similar ultraviolet properties but differing radio properties suggests, perhaps, that the radio and ultraviolet emission is tracing activity occurring on different time-scales.

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