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
Sey 2
D=98.4 Mpc
2MASX J07561963-4137420
Miscellaneous :
Sazonov et al. 2005 :
Masetti et al. 2006 :
  • z=0.021
  • Halpha emission
  • Seyfert2
De Rosa et al. 2008 :
  • Chandra Observation
  • Compton thin AGN
  • NH=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=108.02 MSun and LEdd=1046.12 erg/s
  • LBol=0.008 LEdd

Last updated. 22 Nov. 2012

Jerome Rodriguez