Variable Absorption and Extended X-ray Emission in the BAL RLQ PG 1004+130

Details Variable Absorption and Extended X-ray Emission in the BAL RLQ PG 1004+130 Variable Absorption and Extended X-ray Emission in the BAL RLQ PG 1004+130

Oct 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010xmm..prop..126b&link_type=abstract

XMM-Newton Proposal ID #06730301

Computer Science

Active Galactic Nuclei, Quasars, Bl-Lac Objects, X-Ray Background, Pg 1004+130

Scientific paper

We propose joint XMM-Newton (60 ks) and non-simultaneous Chandra (60 ks) observations of the remarkable BAL RLQ PG 1004+130 which, in conjunction with our previous X-ray coverage, will yield: (1) One of the most comprehensive X-ray spectral monitoring campaigns of a variable BAL quasar undertaken to date, probing both multi-year and multi-month timescales and constraining the location and dynamics of the X-ray absorber. (2) The highest signal-to-noise X-ray spectrum of a BAL RLQ currently available, enabling modeling of soft X-ray absorption and the underlying continuum. (3) The deepest X-ray coverage yet obtained of a disrupting jet in a hybrid morphology radio source, allowing tests for jet flux variability and characterization of the morphologies and spectra of the jet and diffuse emission.

Affiliated with

Also associated with

No associations

Rating

Variable Absorption and Extended X-ray Emission in the BAL RLQ PG 1004+130 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Variable Absorption and Extended X-ray Emission in the BAL RLQ PG 1004+130, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Variable Absorption and Extended X-ray Emission in the BAL RLQ PG 1004+130 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1314390