Table 2: Fits to the 0.2-10 keV X-ray continuum, the Fe K$\alpha $ emission line region and the 0.32-2.07 keV RGS continuum.
\begin{table}\begin{displaymath} \begin{array}{p{0.7in}p{1.2in}p{1.2in}p{1.1i... ...4) \\ \noalign{\smallskip } \hline \end{array} \end{displaymath} \end{table}
$^{\rm {a}}$ Galactic absorbing column in 10$^{\rm 20}$ cm$^{\rm -2}$, fixed (Elvis et al. 1989).
$^{\rm {b}}$ Photon index.
$^{\rm {c}}$ Power-law normalisation in 10$^{\rm -3}$ photons keV$^{\rm -1}$ cm$^{\rm -2}$ s$^{\rm -1}$ at 1 keV.
$^{\rm {d}}$ Temperature of blackbody 1 in keV.
$^{\rm {e}}$ Normalisation of blackbody 1; 10 $^{\rm -4}~L_{39}$/ D102, where L39 is the source luminosity in units of 1039 ergs s$^{\rm -1}$ and  $D_{\rm 10}$ is the distance
to the source in units of 10 kpc.
$^{\rm {f}}$ Temperature of blackbody 2 in keV.
$^{\rm {g}}$ Normalisation of blackbody 2; 10 $^{\rm -5}~L_{39}$/ D102, where L39 is the source luminosity in units of 1039 ergs s$^{\rm -1}$ and  $D_{\rm 10}$ is the distance
to the source in units of 10 kpc.
$^{\rm {h}}$ Measured rest frame energy of the Fe K$\alpha $ line in keV.
$^{\rm {i}}$ FWHM of Fe K$\alpha $ line in eV.
$^{\rm {j}}$ Velocity broadening (FWHM) of Fe K$\alpha $ line in km s$^{\rm -1}$.
$^{\rm {k}}$ Redshifted velocity of Fe K$\alpha $ line in km s$^{\rm -1}$ (negative values indicate blueshifts).
$^{\rm {l}}$ Flux of Fe K$\alpha $ line in 10$^{\rm -5}$ photons cm$^{\rm -2}$ s$^{\rm -1}$.
$^{\rm {m}}$ Reduced $\chi^{\rm 2}$ of the total fit; the degrees of freedom are given in brackets.
$^{\rm {n}}$ In the range 0.2-10 keV.
$^{\rm {o}}$ In the range 5-8 keV.
$^{\rm {p}}$ In the range 0.32-2.07 keV.
$^{\rm {q}}$ Fixed.

Source LaTeX | All tables | In the text