The nature of the ultraluminous X-ray sources inside galaxies and their relation to local QSOs
arXiv:astro-ph/0211139 · doi:10.1051/0004-6361:20030134
Abstract
It is suggested that many of the ultraluminous compact x-ray sources now being found in the main bodies of galaxies, particularly those that are active, like M82, NGC 3628 and others, are "local" QSOs, or BL Lac objects, with high intrinsic redshifts in the process of being ejected from those galaxies. Evidence in support of this hypothesis is summarized.
arXiv commentsubmitted to A&A Letters
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Cited by in corpus (7)
- Optical Counterparts of Ultra Luminous X-ray Sources
- Optical Counterparts of Ultraluminous X-Ray Sources
- New optical spectra and general discussion on the nature of ULX's
- The Discovery of a High Redshift X-ray Emitting QSO Very Close to the Nucleus of NGC 7319
- Toward a Clean Sample of Ultra-Luminous X-ray Sources
- QSOs Associated with Messier 82
- A Test for the Origin of Quasar Redshifts