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- W3101383039 endingPage "22" @default.
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- W3101383039 abstract "Photodissociation regions (PDRs) are parts of the ISM consisting of predominantly neutral gas, located at the interface between H II regions and molecular clouds. The physical conditions within these regions show variations on very short spatial scales, and therefore PDRs constitute ideal laboratories for investigating the properties and evolution of dust grains. We have mapped IC 63 at high resolution from the UV to the NIR (275 nm to 1.6 $mu$m), using the Hubble Space Telescope WFC3. Using a Bayesian SED fitting tool, we simultaneously derive a set of stellar ($T_text{eff}$, $log(g)$, distance) and extinction ($A_V$, $R_V$) parameters for 520 background stars. We present maps of $A_V$ and $R_V$ with a resolution of 25 arcsec based on these results. The extinction properties vary across the PDR, with values for $A_V$ between 0.5 and 1.4 mag, and a decreasing trend in $R_V$, going from 3.7 at the front of the nebula to values as low as 2.5 further in. This provides evidence for evolution of the dust optical properties. We fit two modified blackbodies to the MIR and FIR SED, obtained by combining the $A_V$ map with data from Spitzer and Herschel. We derive effective temperatures (30 K and 227 K) and the ratio of opacities at 160 $mu$m to V band $kappa_{160} / kappa_V$ ($7.0 times 10^{-4}$ and $2.9 times 10^{-9}$) for the two dust populations. Similar fits to individual pixels show spatial variations of $kappa_{160} / kappa_{V}$. The analysis of our HST data, combined with these Spitzer and Herschel data, provides the first panchromatic view of dust within a PDR." @default.
- W3101383039 created "2020-11-23" @default.
- W3101383039 creator A5001375518 @default.
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- W3101383039 date "2019-12-30" @default.
- W3101383039 modified "2023-09-23" @default.
- W3101383039 title "Evidence of Dust Grain Evolution from Extinction Mapping in the IC 63 Photodissociation Region" @default.
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- W3101383039 cites W1904411640 @default.
- W3101383039 cites W1977521416 @default.
- W3101383039 cites W1991028833 @default.
- W3101383039 cites W1999261529 @default.
- W3101383039 cites W2000070292 @default.
- W3101383039 cites W2019579421 @default.
- W3101383039 cites W2020097419 @default.
- W3101383039 cites W2026067008 @default.
- W3101383039 cites W2032348950 @default.
- W3101383039 cites W2035198704 @default.
- W3101383039 cites W2037131602 @default.
- W3101383039 cites W2039874334 @default.
- W3101383039 cites W2044669640 @default.
- W3101383039 cites W2048274049 @default.
- W3101383039 cites W2049089350 @default.
- W3101383039 cites W2072394126 @default.
- W3101383039 cites W2075376439 @default.
- W3101383039 cites W2075683553 @default.
- W3101383039 cites W2085134357 @default.
- W3101383039 cites W2100833883 @default.
- W3101383039 cites W2108706852 @default.
- W3101383039 cites W2109362894 @default.
- W3101383039 cites W2110015992 @default.
- W3101383039 cites W2114246636 @default.
- W3101383039 cites W2115022808 @default.
- W3101383039 cites W2131287406 @default.
- W3101383039 cites W2131965879 @default.
- W3101383039 cites W2135536375 @default.
- W3101383039 cites W2135625048 @default.
- W3101383039 cites W2140137154 @default.
- W3101383039 cites W2145949657 @default.
- W3101383039 cites W2148804397 @default.
- W3101383039 cites W2151413974 @default.
- W3101383039 cites W2161674160 @default.
- W3101383039 cites W2165990266 @default.
- W3101383039 cites W2167635287 @default.
- W3101383039 cites W2178336115 @default.
- W3101383039 cites W2474106573 @default.
- W3101383039 cites W2535532860 @default.
- W3101383039 cites W2688992495 @default.
- W3101383039 cites W2784383761 @default.
- W3101383039 cites W2798336535 @default.
- W3101383039 cites W2888532099 @default.
- W3101383039 cites W2894811230 @default.
- W3101383039 cites W2911198980 @default.
- W3101383039 cites W2963971987 @default.
- W3101383039 cites W3098800005 @default.
- W3101383039 cites W3098836012 @default.
- W3101383039 cites W3099491677 @default.
- W3101383039 cites W3099549426 @default.
- W3101383039 cites W3100106758 @default.
- W3101383039 cites W3100141026 @default.
- W3101383039 cites W3101048891 @default.
- W3101383039 cites W3101187304 @default.
- W3101383039 cites W3101330895 @default.
- W3101383039 cites W3101691828 @default.
- W3101383039 cites W3102117409 @default.
- W3101383039 cites W3102594821 @default.
- W3101383039 cites W3103356242 @default.
- W3101383039 cites W3103460426 @default.
- W3101383039 cites W3103995240 @default.
- W3101383039 cites W3104314891 @default.
- W3101383039 cites W3104917396 @default.
- W3101383039 cites W3105815744 @default.
- W3101383039 cites W3106199679 @default.
- W3101383039 cites W3106253105 @default.
- W3101383039 cites W3122655791 @default.
- W3101383039 cites W3124718545 @default.
- W3101383039 cites W3125590226 @default.
- W3101383039 cites W4289710459 @default.
- W3101383039 cites W4293003757 @default.
- W3101383039 cites W4295004167 @default.
- W3101383039 cites W4297293465 @default.
- W3101383039 cites W4300629171 @default.
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- W3101383039 doi "https://doi.org/10.3847/1538-4357/ab557f" @default.
- W3101383039 hasPublicationYear "2019" @default.
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