All Figures

$\begin{figure} \par\includegraphics[width=8.6cm,clip]{4338fg1a.eps} \includegrap... ....eps} \includegraphics[width=8.4cm,height=5cm,clip]{4338fg1d.eps} \end{figure}$ Figure 1: Upper left: Merlin image of 3C 277.1 at 6 cm and 0.06 $^{\prime \prime }$ resolution, contours are total intensity, vectors have lengths proportional to the bias corrected polarized intensity and the orientation of the E-vectors. Contours are powers of 2 times 200 $\mu$ Jy, negative contours are dashed. The circle in the lower left corner gives the resolution of the image. The image is rotated on the sky by -42 $^\circ$ . Upper right: fractional polarization gray-scale with superposed total intensity contours. fractional polarization scale is shown in the wedge on the top. Contours are powers of 4 times 200 $\mu$ Jy. Lower: like upper but at 0.12 $^{\prime \prime }$ resolution.
Open with DEXTER

In the text

$\begin{figure} \par {\hbox{ \includegraphics[height=9cm,angle=-90]{4338fg2a.eps} \includegraphics[height=9cm,angle=-90]{4338fg2b.eps} }} \end{figure}$ Figure 2: Left: VLA image of 3C 277.1 at 3.6 cm and 0.12 $^{\prime \prime }$ resolution, contours are total intensity, vectors have lengths proportional to the bias corrected polarized intensity and the orientation of the E-vectors. Contours are powers of 2 times 100 $\mu$ Jy, negative contours are dashed. The circle in the lower left corner gives the resolution of the image. The image is rotated by -42 $^\circ$ . Right: fractional polarization gray-scale with superposed total intensity contours. Fractional polarization scale is shown in the wedge on the top. Contours are powers of 4 times 100 $\mu$ Jy.
Open with DEXTER

In the text

$\begin{figure} \par {\hbox{ \includegraphics[height=9cm,angle=-90]{4338fg3a.eps... ...g3c.eps} \includegraphics[height=9cm,angle=-90]{4338fg3d.eps} }} \end{figure}$ Figure 3: Upper: VLA image of 3C 277.1 at 2 cm and 0.06 $^{\prime \prime }$ resolution, contours are total intensity, vectors have lengths proportional to the bias corrected polarized intensity and the orientation of the E-vectors. Contours are powers of 2 times 100 $\mu$ Jy, negative contours are dashed. The circle in the lower left corner gives the resolution of the image. The image is rotated by -42 $^\circ$ . Upper right: fractional polarization gray-scale with superposed total intensity contours. Fractional polarization scale is shown in the wedge on the top. Contours are powers of 4 times 100 $\mu$ Jy. Lower: like upper but at 0.12 $^{\prime \prime }$ resolution.
Open with DEXTER

In the text

$\begin{figure} \par {\hbox{ \includegraphics[height=9cm,angle=-90]{4338fg4a.eps... ....eps} \includegraphics[height=9cm,angle=-90]{4338fg4d.eps} }} \par\end{figure}$ Figure 4: Upper Left: VLA image of 3C 277.1 at 1.3 cm and 0.06 $^{\prime \prime }$ resolution, contours are total intensity, vectors have lengths proportional to the bias corrected polarized intensity and the orientation of the E-vectors. Contours are powers of 2 times 100 $\mu$ Jy, negative contours are dashed. The circle in the lower left corner gives the resolution of the image. The image is rotated by -42 $^\circ$ . Upper right: fractional polarization gray-scale with superposed total intensity contours. Fractional polarization scale is shown in the wedge on the top. Contours are powers of 4 times 100 $\mu$ Jy. Lower: like upper but at 0.12 $^{\prime \prime }$ resolution.
Open with DEXTER

In the text

$\begin{figure} \par {\hbox{ \includegraphics[height=9cm,angle=-90]{4338fig5.eps} }} \end{figure}$ Figure 5: The gray scale shows the rotation measure image at 0.12 $^{\prime \prime }$ resolution with superposed contours of the VLA 3.6 cm image. Rotation measures are in the observer's frame. Plots of the polarization angle as a function of wavelength squared are shown with lines representing the fitted rotation measure for a number of locations. The estimated errors are either given by the vertical size of the cross or are smaller. The bar at the top gives the values of the gray scale in rad m^-2. Contours are powers of 4 times 200 $\mu$ Jy. The circle in the lower left corner gives the resolution. The image is rotated by -42 $^\circ$ .
Open with DEXTER

In the text

$\begin{figure} \par {\hbox{ \includegraphics[height=9cm,angle=-90]{4338fig6.eps} }} \end{figure}$ Figure 6: Contours of the 2 cm 0.12 $^{\prime \prime }$ resolution image with vectors whose length are proportional to the 2 cm fractional polarization and the derived intrinsic polarization angle. Contours are powers of 2 times 200 $\mu$ Jy. The image is rotated by -42 $^\circ$ .
Open with DEXTER

In the text

$\begin{figure} \par {\hbox{ \includegraphics[height=9cm,angle=-90]{4338fg7a.eps... ...{\hbox{ \includegraphics[height=9cm,angle=-90]{4338fg7c.eps} }} \end{figure}$ Figure 7: Top: the gray scale shows the ratio of the fractional polarization at 6 cm to that at 1.3 cm with superposed contours of the 2 cm 0.12 $^{\prime \prime }$ resolution image. Contours are powers of 4 times 100 $\mu$ Jy. The image is rotated by -42 $^\circ$ . Middle: like top but the ratio of 3.6 to 1.3 cm fractional polarizations. Bottom: like top but the ratio of 6 to 1.3 cm fractional polarizations.
Open with DEXTER

In the text

$\begin{figure} \par {\hbox{ \includegraphics[height=9cm,angle=-90]{4338fig8.eps} }} \end{figure}$ Figure 8: The gray scale shows the spectral index at 0.12 $^{\prime \prime }$ resolution between 6 and 1.3 cm with superposed contours of the 2 cm 0.12'' resolution image. Contours are powers of 4 times 100 $\mu$ Jy. The image is rotated by -42 $^\circ$ .
Open with DEXTER

In the text

$\begin{figure} \par {\hbox{ \includegraphics[height=9cm,angle=-90]{4338fg9a.eps... ...{\hbox{ \includegraphics[height=9cm,angle=-90]{4338fg9b.eps} }} \end{figure}$ Figure 9: Results of pixel-by-pixel fitting of Burn (1966) model at 0.12 $^{\prime \prime }$ resolution. Top: the gray scale shows the derived fractional polarization at zero wavelength with superposed contours of the 3.6 cm total intensity image. Contours are powers of 4 times 200 $\mu$ Jy; the gray scale values are indicated by the wedge at the top. The image is rotated by -42 $^\circ$ . Bottom: the gray scale gives the derived Faraday dispersion ( $\sigma$ ) in rad/ ${\rm m^2}$ . Shown below is the fractional polarization as a function of wavelength squared for selected locations represented as pluses (+). The solid line is the fitted model, errors equal or are less than the vertical extent of the pluses.
Open with DEXTER

In the text

$\begin{figure} \par {\hbox{ \includegraphics[width=9cm]{4338fg10.eps} }} \end{figure}$ Figure 10: Negative gray scale of the O[III] emission image with superposed contours of the VLA 3.6 cm image. The bar at the top gives the values of the gray scale. Contours are powers of 4 times 200 $\mu$ Jy. The circle in the lower left corner gives the resolution of the 3.6 cm image. The images are rotated by -42 $^\circ$ .
Open with DEXTER

In the text

$\begin{figure} \par {\hbox{ \includegraphics[width=6cm,angle=-90]{4338fg11.eps} }} \end{figure}$ Figure 11: Fitted spectral decomposition with only synchrotron opacity for all components. Fitted data are shown with vertical error bars. The solid line is the total model flux density and the dashed lines are individual component spectra, "C'' = core, "W'' = west lobe, "E'' = east lobe. The west lobe has its low frequency cutoff around 1 GHz, the core has a flat spectrum and the east component has a low frequency cutoff around 0.06 GHz.
Open with DEXTER

In the text

$\begin{figure} \par {\hbox{ \includegraphics[width=6cm,angle=-90]{4338fg12.eps} }} \end{figure}$ Figure 12: Fitted spectral decomposition with only free-free opacity in the east lobe and only synchrotron opacity for the other components. Fitted data are shown with vertical error bars. The solid line is the total model flux density and the dashed lines are individual component spectra, "C''=core, "W'' = west lobe, "E'' = east lobe. The west lobe has its low frequency cutoff around 1 GHz, the core has a flat spectrum and the east component has a low frequency cutoff around 0.06 GHz.
Open with DEXTER

In the text

$\begin{figure} \par {\hbox{ \includegraphics[width=6cm,angle=-90]{4338fg13.eps} }}\end{figure}$ Figure 13: Scatter plot of the radio continuum at 3.6 cm versus the [OIII] emission on a pixel-by-pixel basis of the images shown in Fig. 10 but excluding the nuclear region. Brightnesses are given in arbitrary units. The near anti-correlation is shown by the "L'' shape of the distribution.
Open with DEXTER

In the text

$\begin{figure} \par {\hbox{ \includegraphics[height=9cm]{4338f14a.eps} \includegraphics[height=9cm]{4338f14b.eps} }} \end{figure}$ Figure 14: Left: closeup of east lobe of 3C 277.1 with the intrinsic polarization (m₀ from Burn model fit to 0.12 $^{\prime \prime }$ resolution data) in negative gray-scale and the HST [OIII] emission as contours. The decreasing polarization fraction toward the region of [OIII] emission is readily apparent. The scale of the intrinsic polarization is given by the wedge at the top. The [OIII] contour are factors of $\sqrt {2}$ and are arbitrary units The image is rotated by -42 $^\circ$ . Right: same area as left but showing 1.3 cm 0.06 $^{\prime \prime }$ resolution bias corrected polarized intensity as grayscale and total intensity as contours. The gray-scale is given in mJy by the wedge at the top; contours are are factors of $\sqrt {2}$ times 0.5 mJy.
Open with DEXTER

In the text

$\begin{figure} \par {\hbox{ \includegraphics[height=9cm,angle=-90]{4338fig6.eps} }} \end{figure}$	Figure 6: Contours of the 2 cm 0.12 $^{\prime \prime }$ resolution image with vectors whose length are proportional to the 2 cm fractional polarization and the derived intrinsic polarization angle. Contours are powers of 2 times 200 $\mu$ Jy. The image is rotated by -42 $^\circ$ .
Open with DEXTER

$\begin{figure} \par {\hbox{ \includegraphics[height=9cm,angle=-90]{4338fig8.eps} }} \end{figure}$	Figure 8: The gray scale shows the spectral index at 0.12 $^{\prime \prime }$ resolution between 6 and 1.3 cm with superposed contours of the 2 cm 0.12'' resolution image. Contours are powers of 4 times 100 $\mu$ Jy. The image is rotated by -42 $^\circ$ .
Open with DEXTER

$\begin{figure} \par {\hbox{ \includegraphics[width=9cm]{4338fg10.eps} }} \end{figure}$	Figure 10: Negative gray scale of the O[III] emission image with superposed contours of the VLA 3.6 cm image. The bar at the top gives the values of the gray scale. Contours are powers of 4 times 200 $\mu$ Jy. The circle in the lower left corner gives the resolution of the 3.6 cm image. The images are rotated by -42 $^\circ$ .
Open with DEXTER

$\begin{figure} \par {\hbox{ \includegraphics[width=6cm,angle=-90]{4338fg13.eps} }}\end{figure}$	Figure 13: Scatter plot of the radio continuum at 3.6 cm versus the [OIII] emission on a pixel-by-pixel basis of the images shown in Fig. 10 but excluding the nuclear region. Brightnesses are given in arbitrary units. The near anti-correlation is shown by the "L'' shape of the distribution.
Open with DEXTER