red=radio, blue=X-ray, green=optical (Fig. RGB)
big image
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| minicon short
agenda |
minicon full
list of questions |
draft paper
(ps) |
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| (jump to
comparisons section) |
red=radio, blue=X-ray, green=optical (Fig. RGB) big image |
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 HST WFPC2 three color composite (red=F850LP [SIII],green=F675W,blue=F450W [OIII]) (Fig. 2A) big image |
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 VLA 6 cm radio polarized intensity big image |
 VLA 6 cm radio (Fig. 1) big image |
 Chandra 0.3-10 keV X-ray (broadband) (Fig. 4) big image |
 Chandra continuum dominated X-ray emission (4-6 keV with Si line emission subtraction) (Fig. 6) big image |
 Chandra FeL+Ne dominated X-ray emission (relative to cont.) (0.85-1.0 keV with high energy continuum subtraction) This energy range also includes Ne IX emission and may contain some O VII and Ne X emission due to the energy resolution of the ACIS-S3 chip big image |
 Chandra Si dominated X-ray emission (relative to continuum) (1.72-1.96 keV with high energy [4-6 keV] continuum subtraction) (Fig. 14) This energy range also includes Al and Mg emission big image |
 Chandra Fe K dominated X-ray emission (relative to cont.) (6.2-6.92 keV with high energy continuum subtraction) This energy range only includes Fe emission big image |
 Chandra S dominated X-ray emission (relative to cont.) (2.29-2.58 keV with high energy continuum subtraction) This energy range also includes Si emission big image |
 Chandra O dominated X-ray emission (relative to cont.) (0.64-0.71 keV with high energy continuum subtraction) This energy range may include Ca and Fe emission due to the energy resolution of the ACIS-S3 chip (Fig. 18) big image |
 VLA flat-spectrum radio image big image |
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| X-ray
Si and S Compared to Optical S |
X-ray
O Compared to Optical O |
| X-ray FeL+Ne
Compared to Optical QSF |
Continuum
X-rays and Radio Emission |
| Southern
Bowshock Region |
Northwest
Reverse Shock Region |
| Proper
Motions |
X-ray Si
and Flat-Spectrum Radio |
| Diffuse
Halpha |
Absorption
(XMM) |
| Tomography |
