IGR J14552-5133

	IGR J14552-5133


	Other name = WKK 4488

Type	redshift	Radio Counterpart			Infrared/Optical Counterpart
		R.A. (J2000)	Dec. (J2000)	References	R.A. (J2000)	Dec. (J2000)	References
AGN Narrow line Sey 1	0.016 d=74.7 Mpc
References		Revnivtsev et al. 2005 astro-ph0508155 Masetti et al. 2006, A&A, 459, 21 Malizia et al. 2007, ApJ, 668,81 Malizia et al. 2008, MNRAS, 389, 1360 Panessa et al. 2011, accepted in MNRAS arXiV 1106.3023 Khorunzhev et al. 2012 Astr. Lett., 38, 475

Miscellaneous :

Masetti et al. 2006 :

NL Sey 1
z=0.016
Hbeta, OIII emission lines

Landi et al. 2007: ATel 990

Refinement of the position with Swift XRT
Confirm the association of the X-ray source with the Sey 1 galaxy
absorbed power law spectrum Gamma=2.06 N_H=1.2 x 10²¹ cm^-2
2-10 keV flux of 9e-12 erg/cm2/s

Malizia et al. 2008:

Swift/XRT and INTEGRAL/IBIS/ISGRI broad band spectral analysis
Variability at soft X-rays
Absorbed power law (Γ=1.93), Absorbed cut off pl (Γ=1.88, Ec=46 keV), absorbed broken pl (Γ₁=1.92, Eb=50 keV, Γ₂ unconstrained) fit the data well.
N_H compatible with Galactic absorption

Khorunzev et al. 2012:

Etimate of mass and accretion rate based on different methods
Correltion with bulge luminosity => M = 10^7.23 M_Sun and L_Edd = 10^45.33 erg/s
L_Bol=0.033 L_Edd

Last updated 22 Nov 2012

Jerome Rodriguez