The BeppoSAX observations of the bright Narrow-Line Seyfert I galaxy Ark 564 are presented along with a high quality optical spectrum taken at the 1.5 m telescope at La Silla. The 0.1-10 keV X-ray spectrum is characterized by a strong soft; component which is best described by blackbody-like emission with a temperature of similar to 160 eV. At higher energies a steep (Gamma similar or equal to 2.4) power-law tail is present. There is evidence of an ionized reflector in the form of an iron line and edge. We do not find significant evidence of soft X-ray features if the spectrum is modelled with a two component continuum. The optical and X-ray spectral properties support the hypothesis of a high accretion rate onto a low mass black hole.
Comastri, A., Stirpe, G.m., Vignali, C., Brandt, W.n., Leighly, K.m., Fiore, F., et al. (2001). BeppoSAX observations of Narrow-Line Seyfert 1 galaxies - II. Ionized iron features in Arakelian 564. ASTRONOMY & ASTROPHYSICS, 365(3), 400-408.
BeppoSAX observations of Narrow-Line Seyfert 1 galaxies - II. Ionized iron features in Arakelian 564
MATT, Giorgio;
2001-01-01
Abstract
The BeppoSAX observations of the bright Narrow-Line Seyfert I galaxy Ark 564 are presented along with a high quality optical spectrum taken at the 1.5 m telescope at La Silla. The 0.1-10 keV X-ray spectrum is characterized by a strong soft; component which is best described by blackbody-like emission with a temperature of similar to 160 eV. At higher energies a steep (Gamma similar or equal to 2.4) power-law tail is present. There is evidence of an ionized reflector in the form of an iron line and edge. We do not find significant evidence of soft X-ray features if the spectrum is modelled with a two component continuum. The optical and X-ray spectral properties support the hypothesis of a high accretion rate onto a low mass black hole.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
