IGR J07565-4139

	IGR J07565-4139


	Other name = IGR J07563-4137

Type	redshift	Radio Counterpart			Infrared/Optical Counterpart
		R.A. (J2000)	Dec. (J2000)	References	R.A. (J2000)	Dec. (J2000)	References
AGN Sey 2	0.021 D=98.4 Mpc				2MASX J07561963-4137420
References		Bird et al. 2006 ApJ, 636, 765 Sazonov et al. 2005 A&A A&A, 444, L37 Masetti et al. 2006, A&A, 459, 21 Malizia et al. 2007, ApJ, 668,81 De Rosa et al. 2008, A&A, 483, 749 De Rosa et al. 2012, MNRAS, 420, 2087 Khorunzhev et al. 2012 Astr. Lett., 38, 475

Miscellaneous :

Sazonov et al. 2005 :

nH=(1.1+/-0.2)x10^22

Masetti et al. 2006 :

z=0.021
Halpha emission
Seyfert2

De Rosa et al. 2008 :

Chandra Observation
Compton thin AGN
N_H=0.4 x 10²² cm^-2 with phenomenological model
Possible presence of a high energy cut-off of 40_-10⁺¹⁶⁰ keV
Source is peculiar, best fit model: absorbed e-folded power law, reflection (upper limit on reflection), and thermal sof emission
Narrow 2.46 keV with 184 eV EW required in the fit

Khorunzev et al. 2012:

Etimate of mass and accretion rate based on different methods
Correltion with bulge luminosity => M=10^8.02 M_Sun and L_Edd=10^46.12 erg/s
L_Bol=0.008 L_Edd

Last updated. 22 Nov. 2012

Jerome Rodriguez