The radio structure of the peculiar narrow-line Seyfert 1 galaxy candidate J1100+4421

Tutkimustuotos: Lehtiartikkelivertaisarvioitu

Tutkijat

Organisaatiot

  • Hungarian Academy of Sciences
  • Joint Institute for VLBI in Europe
  • University of Tokyo
  • Chinese Academy of Sciences
  • National Astronomical Observatory of Japan
  • Eotvos Lorand University

Kuvaus

Narrow-line Seyfert 1 galaxies (NLS1) are an intriguing subclass of active galactic nuclei. Their observed properties indicate low central black hole mass and high accretion rate. The extremely radio-loud NLS1 sources often show relativistic beaming and are usually regarded as younger counterparts of blazars. Recently, the object SDSS J110006.07+442144.3 was reported as a candidate NLS1 source. The characteristics of its dramatic optical flare indicated its jet-related origin. The spectral energy distribution of the object was similar to that of the γ-ray detected radio-loud NLS1, PMN J0948+0022. Our high-resolution European very long baseline interferometry network observations at 1.7 and 5 GHz revealed a compact core feature with a brightness temperature of ≳1010 K. Using the lowest brightness temperature value and assuming a moderate Lorentz factor of ∼9, the jet viewing angle is ≲26°. Archival Very Large Array data show a large-scale radio structure with a projected linear size of ∼150 kpc reminiscent of double-sided morphology.

Yksityiskohdat

AlkuperäiskieliEnglanti
Sivut1554-1561
Sivumäärä8
JulkaisuMonthly Notices of the Royal Astronomical Society
Vuosikerta473
Numero2
TilaJulkaistu - 11 tammikuuta 2018
OKM-julkaisutyyppiA1 Julkaistu artikkeli, soviteltu

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