IGR J12026-5349

	IGR J12026-5349


	Other name = WKK 0560

Type	Redshift	Radio Counterpart			Infrared/Optical Counterpart
		R.A. (J2000)	Dec. (J2000)	References	R.A. (J2000)	Dec. (J2000)	References
AGN Sey 2	0.028 d=131.4 Mpc
References		Revnivtsev et al. 2005 astro-ph0508155 Sazonov et al. 2005 A&A, 444, L37 Masetti et al. 2006, A&A, 459, 21 De Rosa et al. 2008A&A, 483, 749 Winter et al. 2009, ApJ, 690, 1322 De Rosa et al. 2012,MNRAS, 420, 2087 Khorunzhev et al. 2012 Astr. Lett., 38, 475

Miscellaneous :

Sazonov et al. 2005 :

z=0.0280, nH=(2.2+/-0.3)x10^22

Masetti et al. 2006 :

Halpha, Hbeta, OIII emission lines
Sey 2

De Rosa et al. 2008 :

Chandra Observation
Unabsorbed soft excess on top of absorbed power law + Gaussian @ 6.4 keV
High value of kT compared to typical Sey 2 (1.2 keV)
Not scattered component at the origin of soft excess, but possibly starbust
Compton thin AGN
N_H=31 x 10²² cm^-2 with phenomenological model
High energy cut-off of 170_-50⁺¹³⁰ keV, possible reflection feature

Winter et al. 2009:

Host galaxy is a SB0 pec, Int (as obtained from NED)

Khorunzev et al. 2012:

Etimate of mass and accretion rate based on different methods
Correltion with bulge luminosity => M = 10^8.20 M_Sun and L_Edd = 10^46.30 erg/s
L_Bol=0.019 L_Edd

Last updated. 22 Nov 2012

Jerome Rodriguez