2002A&A...385L..31B

Query : 2002A&A...385L..31B

2002A&A...385L..31B - Astronomy and Astrophysics, volume 385, L31-35 (2002/4-3)

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

BRINKMANN W., FERRERO E. and GLIOZZI M.

Abstract (from CDS):

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 >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.

Abstract Copyright: ∼

Journal keyword(s): galaxies: active - quasars - X-rays: galaxies

Simbad objects: 6

Full paper

View the references in ADS

Number of rows : 6

N	Identifier	Otype	ICRS (J2000) RA	ICRS (J2000) DEC	Mag B	Mag V	Mag R	Sp type	#ref 1850 - 2023
1	LEDA 50824	Sy1	14 13 48.3306274368	+44 00 14.003371296	14.99	14.99		~	378
2	NAME phl5200-001	AGN	22 28 26.4	-05 18 19			21.21	~	5
3	QSO B2225-055	QSO	22 28 30.3464915928	-05 18 54.694692252	18.45	17.70		~	157
4	[GS80] PHL 5200 A	Rad	~	~				~	2
5	[GS80] PHL 5200 B	Rad	~	~				~	2
6	[GS80] PHL 5200 C	Rad	~	~				~	2

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