XMM-Newton observation of the BAL Quasar PHL 5200:. The big surprise

Details XMM-Newton observation of the BAL Quasar PHL 5200:. The big surprise XMM-Newton observation of the BAL Quasar PHL 5200:. The big surprise

Apr 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002a%26a...385l..31b&link_type=abstract

Astronomy and Astrophysics, v.385, p.L31-L35 (2002)

Astronomy and Astrophysics

Astrophysics

7

Galaxies: Active, Quasars, X-Rays: Galaxies

Scientific paper

XMM-Newton observations of the BAL quasar PHL 5200 revealed that the X-ray emission attributed to the quasar originates from a nearby, optically unidentified radio source. Although visible in X-rays as well the flux from PHL 5200 is by a factor ga 20 smaller than previously anticipated. Thus most of the scenarios for a physical interpretation of the BAL phenomenon, based on the apparently unexpected X-ray properties of this quasar have to be revisited. We further discuss the properties of the optically very faint radio source.

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