Suzaku Results on the Obscured Low-Luminosity Active Galactic Nucleus in NGC 4258
arXiv:0812.0145 · doi:10.1093/pasj/61.2.309
Abstract
In 2006 June, the obscured low luminosity active galactic nucleus in the nearby Seyfert 1.9 galaxy NGC 4258 was observed with Suzaku for ~ 100 ks. Utilizing the XIS and the HXD, the nucleus emission was detected over 2 to 40 keV range, with an unabsorbed 2--10 keV luminosity of 8 x 10 40 erg / s, and varied by a factor of ~ 2 during the observation. Its 2--40 keV spectrum is reproduced by a single power law with photon index of ~ 2.0, absorbed by an equivalent hydrogen column of ~ 1.0 x 10 23 cm2. The spectrum within 4' of the nucleus required also a softer thin-thermal emission, as well as an intermediate hardness component attributable to integrated point sources. A weak neutral Fe-Kalpha florescence line was detected at an equivalent width of ~ 40 eV. The cold reflection component was not required by the data, with the reflector solid angle Omega seen from the nucleus constrained as Omega / 2 pi < 0.3 assuming a general case of 60 deg inclination. The results suggest that the cold reflecting material around the nucleus is localized along our line of sight, rather than forming a thick torus.
PASJ, NGC4258, Suzaku, 12 pages, 11 figures
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- The INTEGRAL/IBIS AGN catalogue I: X-ray absorption properties versus optical classification
- Long-term X-Ray Spectral Variability in AGN from the Palomar sample observed by Swift
- Suzaku Studies of Wide-Band Spectral Variability of the Bright Type I Seyfert Galaxy Markarian 509
- New Compton-thick AGN in the circumnuclear water maser hosts UGC3 789 and NGC 6264
- X-ray spectra of hot accretion flows
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- On the role and origin of nonthermal electrons in hot accretion flows
- Suzaku Observation of the Metallicity in the Interstellar Medium of NGC 4258
- The flare model for X-ray variability of NGC 4258
- Hot accretion flows in low-luminosity active galactic nuclei in NGC 4258 and NGC 7213