TY - JOUR
T1 - ROSAT monitoring of persistent giant and rapid variability in the narrow-line Seyfert 1 galaxy IRAS 13224-3809
AU - Boller, Th
AU - Brandt, W. N.
AU - Fabian, A. C.
AU - Fink, H. H.
PY - 1997
Y1 - 1997
N2 - We report evidence for persistent giant and rapid X-ray variability in the radio-quiet, ultrasoft, strong Fe II, narrow-line Seyfert 1 galaxy IRAS 13224-3809. Within a 30-d ROSAT High Resolution Imager (HRI) monitoring observation at least five giant-amplitude count rate variations are visible, with the maximum observed amplitude of variability being about a factor of 60. We detect a rise by a factor of about 57 in just 2 d. IRAS 13224-3809 appears to be the most X-ray-variable Seyfert known, and its variability is probably non-linear. We carefully check the identification of the highly variable X-ray source with the distant galaxy, and it appears to be secure. We examine possible explanations for the giant variability. Unusually strong relativistic effects and partial covering by occulting structures on an accretion disc can provide plausible explanations of the X-ray data, and we explore these two scenarios. Relativistic boosting effects may be relevant to understanding the strong X-ray variability of some steep-spectrum Seyferts more generally.
AB - We report evidence for persistent giant and rapid X-ray variability in the radio-quiet, ultrasoft, strong Fe II, narrow-line Seyfert 1 galaxy IRAS 13224-3809. Within a 30-d ROSAT High Resolution Imager (HRI) monitoring observation at least five giant-amplitude count rate variations are visible, with the maximum observed amplitude of variability being about a factor of 60. We detect a rise by a factor of about 57 in just 2 d. IRAS 13224-3809 appears to be the most X-ray-variable Seyfert known, and its variability is probably non-linear. We carefully check the identification of the highly variable X-ray source with the distant galaxy, and it appears to be secure. We examine possible explanations for the giant variability. Unusually strong relativistic effects and partial covering by occulting structures on an accretion disc can provide plausible explanations of the X-ray data, and we explore these two scenarios. Relativistic boosting effects may be relevant to understanding the strong X-ray variability of some steep-spectrum Seyferts more generally.
UR - http://www.scopus.com/inward/record.url?scp=0002539098&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=0002539098&partnerID=8YFLogxK
U2 - 10.1093/mnras/289.2.393
DO - 10.1093/mnras/289.2.393
M3 - Article
AN - SCOPUS:0002539098
SN - 0035-8711
VL - 289
SP - 393
EP - 405
JO - Monthly Notices of the Royal Astronomical Society
JF - Monthly Notices of the Royal Astronomical Society
IS - 2
ER -