Evidence for an ionised disc in the narrow-line Seyfert 1 galaxy Ark 564
| dc.creator | Vaughan, S. | |
| dc.creator | Pounds, K. A. | |
| dc.creator | Reeves, J. | |
| dc.creator | Warwick, R. | |
| dc.creator | Edelson, R. | |
| dc.date | 1999-06-28 | |
| dc.date | 1999-08-27 | |
| dc.date.accessioned | 2026-07-07T02:32:13Z | |
| dc.date.available | 2026-07-07T02:32:13Z | |
| dc.description | We present simultaneous ASCA and RXTE observations of Ark 564, the brightest known ``narrow-line'' Seyfert 1 in the 2-10 keV band. The measured X-ray spectrum is dominated by a steep (Gamma~2.7) power-law continuum extending to at least 20 keV, with imprinted Fe K-line and -edge features and an additional ``soft excess'' below ~1.5 keV. The energy of the iron K-edge indicates the presence of highly ionised material, which we identify in terms of reflection from a strongly irradiated accretion disc. The high reflectivity of this putative disc, together with its strong intrinsic O VIII Ly-alpha and O VIII recombination emission, can also explain much of the observed soft excess flux. Furthermore, the same spectral model also provides a reasonable match to the very steep 0.1-2 keV spectrum deduced from ROSAT data. The source is much more rapidly variable than ``normal'' Seyfert 1s of comparable luminosity, increasing by a factor of ~50% in 1.6 hours, with no measurable lag between the 0.5-2 keV and 3-12 keV bands, consistent with much of the soft excess flux arising from reprocessing of the primary power-law component in the inner region of the accretion disc. We note, finally, that if the unusually steep power-law component is a result of Compton cooling of a disc corona by an intense soft photon flux, then the implication is that the bulk of these soft photons lie in the unobserved extreme ultraviolet. | |
| dc.description | 5 pages, 4 figures, accepted for publication in MNRAS Letters | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9906445 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9906445 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/14428 | |
| dc.subject | Astrophysics | |
| dc.title | Evidence for an ionised disc in the narrow-line Seyfert 1 galaxy Ark 564 | |
| dc.type | text |