Publication Date:
2014-04-25
Description:
We present SDSS J143244.91+301435.3, a new case of a radio-loud narrow-line Seyfert 1 (RL NLS1) with a relatively high radio power ( P 1.4 GHz = 2.1 10 25 W Hz –1 ) and large radio-loudness parameter ( R 1.4 = 600 ± 100). The radio source is compact with a linear size below ~1.4 kpc but, in contrast to most of the RL NLS1 discovered so far with such a high R 1.4 , its radio spectrum is very steep (α = 0.93, S –α ) and does not support a ‘blazar-like’ nature. Both the small mass of the central supermassive black hole and the high accretion rate relative to the Eddington limit estimated for this object (3.2 10 7 M and 0.27, respectively, with a formal error of ~0.4 dex for both quantities) are typical of the NLS1 class. Through modelling the spectral energy distribution of the source, we have found that the galaxy hosting SDSS J143244.91+301435.3 is undergoing quite intense star formation (SFR = 50 M yr –1 ), which, however, is expected to contribute only marginally (~1 per cent) to the observed radio emission. The radio properties of SDSS J143244.91+301435.3 are remarkably similar to those of compact steep-spectrum (CSS) radio sources, a class of active galactic nuclei (AGN) mostly composed of young radio galaxies. This may suggest a direct link between these two classes of AGN, with CSS sources possibly representing the misaligned version (the so-called ‘parent population’) of RL NLS1 showing blazar characteristics.
Print ISSN:
0035-8711
Electronic ISSN:
1365-2966
Topics:
Physics
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