IGR J18559+1535

	IGR J18559+1535


	Other name = 2E 1853.7+1534, 1RXH J185600.4+153757

Type	Redshift	Radio Counterpart			Infrared/Optical Counterpart
		R.A. (J2000)	Dec. (J2000)	References	R.A. (J2000)	Dec. (J2000)	References
AGN, Seyfert 1	z=0.084				2MASS J18560056+1537584		Rodriguez et al. 2008
Published papers		Masetti et al. 2006, A&A, 448, 547 Bikmaev et al. 2006 Astron. Lett., 32, 221 Sazonov et al. 2007 A&A, 462, 57 Rodriguez et al. 2008, A&A, 482, 731 Khorunzhev et al. 2012 Astr. Lett., 38, 475

Miscellaneous :

Bikmaev et al. 2006 : z=0.0844, Sey 1

Masetti et al. 2006: (A&A)

association with Rosat source
Optical spectrum
Several lines
z=0.084±0.01

Rodriguez et al. 2008:

Refined X-ray position consistent with optical position of Bikmaev et al. 2006
Strongly suggest X-ray source is indeed a Sey 1
J=13.369, H=12.584, K=11.438
m_UVM2>19.4; m_UVW2>20.2
Absorbed power law fits 0.5-9 keV spectra well, Γ= 1.6 N_H=0.7 x10²²cm^-2; F_{2-10 keV}=1.4x 10^-11 erg/s/cm2

Khorunzev et al. 2012:

Etimate of mass and accretion rate based on different methods
Correltion with bulge luminosity => M ≤~ 10^8.35 M_Sun and L_Edd ≤~ 10^46.45 erg/s
L_Bol ≥~ 0.122 L_Edd

Last updated. 22 Nov. 2012

Jerome Rodriguez