Ultrasoft AGN have low velocity (2000 kms-1) broad line
clouds and high variability characteristic of NLS1's. REJ2248-511 is also an
ultrasoft AGN, but its broad lines have FWHM approx. 3000 kms-1 more typical of a
normal Seyfert 1 galaxy. This is the only ultrasoft AGN which does not appear
to follow the otherwise eunanymous trend.
Previous observations in the optical, EUV and X-ray have shown that this
EUV-bright AGN is highly variable across the entire observed spectrum. Here we
present the results of the recent XMM-Newton observation.
The X-ray continuum consists of a variable ultrasoft excess superimposed on a hard power
law. Between the ROSAT and ASCA observations the ultrasoft component completely
disappeared and now we find that it has returned. While we know that the
soft X-ray spectrum shows large amplitude variability on
timescales of a few years at most, the hard power law remains relatively stable
between the ASCA and XMM observations.
We also present near-simultaneous optical spectrophotometry and IR photometry
to constrain the multiwavelength spectral shape.
Previous optical spectra showed that the continuum slope decreased dramatically
becoming much redder in a one year period, indicating a change in strength of
the big blue bump with no change in the BLR line strengths and
velocities. Eight years on from the last observation we find the optical continuum slope rises toward the blue once more, as measured in 1991, with no marked change in the line profiles.
As this AGN is unusual among ultrasoft objects REJ2248-511 is an ideal test
case which we will use in future work to examine the relationship between the
BLR and the incident ionizing continuum.
A deeper probe of the 0.3-2.1 keV spectrum has been made with the high
resolution XMM RGS, simultaneous with the presented EPIC data, to allow
identification of spectral lines and complex absorption features. This XMM
observation was just the first in a series of 3 designed to monitor the
variability of the soft X-ray spectrum.
REJ2248-511 is a challenging source to understand; the most unconventional of
the ultrasoft sources which are themselves poorly understood. However, with a
significant amount of new data still to come the situation for this object
looks promising.
CATEGORY:
ACTIVE GALAXIES AND QUASARS