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X-ray Variability as a Probe of Advection-Dominated Accretion in Low-Luminosity AGN | A. Ptak
; T. Yaqoob
; R. Mushotzky
; P. Serlemitsos
; R. Griffiths
; | Date: |
29 Apr 1998 | Subject: | astro-ph | Abstract: | As a class, LINERs and Low-Luminosity AGN tend to show little or no significant short-term variability (i.e., with time-scales less than a day). This is a marked break for the trend of increased variability in Seyfert 1 galaxies with decreased luminosity. We propose that this difference is due to the lower accretion rate in LINERs and LLAGN which is probably causing the accretion flow to be advection-dominated. This results in a larger characteristic size for the X-ray producing region than is the case in ``normal’’ AGN. Short-term variability may be caused by a localized instability or occultation events, but we note that such events would likely be accompanied by broad-band spectral changes. Since the ADAF is more compact in a Kerr metric, it is possible that the X-ray emission from ADAFs around rotating blackholes would be more variable than X-ray emission from ADAFs in a Schwarzchild metric. Similar variability arguments also apply to other wavelengths, and accordingly multiwavelength monitoring of LLAGN could serve to ``map’’ the ADAF regions. | Source: | arXiv, astro-ph/9804327 | Services: | Forum | Review | PDF | Favorites |
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