XMM-Newton Observation of HE1029-1401; The Variability of the Fe Emission Line.

Details XMM-Newton Observation of HE1029-1401; The Variability of the Fe Emission Line. XMM-Newton Observation of HE1029-1401; The Variability of the Fe Emission Line.

Sep 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006head....9.0749b&link_type=abstract

American Astronomical Society, HEAD meeting #9, #7.49; Bulletin of the American Astronomical Society, Vol. 38, p.357

Astronomy and Astrophysics

Astronomy

Scientific paper

One of the current open questions in high energy studies of AGN is on the Fe emission line and its apparent lack of variability.
Indeed only in a very few examples has a correlation been found between the highly variable continuum and the line flux.
Here we report the results of an XMM-Newton observation of the low redshift QSO HE1029-1401. During this observation the source has shown variability in the Fe emission line, both in its strength and ionization state.

Affiliated with

Also associated with

No associations

Rating

XMM-Newton Observation of HE1029-1401; The Variability of the Fe Emission Line. 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 XMM-Newton Observation of HE1029-1401; The Variability of the Fe Emission Line., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and XMM-Newton Observation of HE1029-1401; The Variability of the Fe Emission Line. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-777183