Discovery of a Binary Active Galactic Nucleus in the Ultraluminous Infrared Galaxy NGC 6240 Using Chandra
Max Planck Society · Max Planck Institute for Extraterrestrial Physics · +2 more institutions
Abstract
Ultraluminous infrared galaxies (ULIRGs) are outstanding due to their huge luminosity output in the infrared, which is predominantly powered by super starbursts and/or hidden active galactic nuclei (AGN). NGC 6240 is one of the nearest ULIRGs and is considered a key representative of its class. Here, we report the first high-resolution imaging spectroscopy of NGC 6240 in X-rays. The observation, performed with the ACIS-S detector aboard the Chandra X-ray observatory, led to the discovery of two hard nuclei, coincident with the optical-IR nuclei of NGC 6240. The AGN character of both nuclei is revealed by the detection of absorbed hard, luminous X-ray emission and two strong neutral Fe_K_alpha lines. In…
Citation impact
- FWCI
- 16.84
- Percentile
- 100%
- References
- 23
Authors
6- SKS. KomossaCorresponding
Max Planck Society, Max Planck Institute for Extraterrestrial Physics
- VBV. Burwitz
Max Planck Institute for Extraterrestrial Physics, Max Planck Society
- GHG. Hasinger
Max Planck Institute for Extraterrestrial Physics, Max Planck Society
- PPP. Predehl
Max Planck Institute for Extraterrestrial Physics, Max Planck Society
- JSJ. S. Kaastra
SRON Netherlands Institute for Space Research
Topics & keywords
- Physics
- Astrophysics
- Active galactic nucleus
- Luminous infrared galaxy
- Galaxy
- Luminosity
- Astronomy
- Infrared
- Affordable and clean energy