Modelling peculiar extinction curves
We investigate the remarkable variety of IR-through-UV extinction curves by modelling extinction profiles with core-mantle grains and a collection of single and stacked polycyclic aromatic hydrocarbons. Such a model can closely reproduce the observed curves, by simply assuming a different ratio of t...
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| Published in | Monthly notices of the Royal Astronomical Society Vol. 410; no. 3; pp. 1932 - 1938 |
|---|---|
| Main Authors | , , , |
| Format | Journal Article |
| Language | English |
| Published |
Oxford, UK
Blackwell Publishing Ltd
01.01.2011
Wiley-Blackwell Oxford University Press |
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| Abstract | We investigate the remarkable variety of IR-through-UV extinction curves by modelling extinction profiles with core-mantle grains and a collection of single and stacked polycyclic aromatic hydrocarbons. Such a model can closely reproduce the observed curves, by simply assuming a different ratio of the molecular component to classical dust, while leaving relatively unmodified the underlying global picture. In particular, we find that for extinction curve morphologies differing significantly from the average Galactic extinction, dust grain sizes exhibit a low-end cut-off at approximately 100 nm. An additional component of very small grains of sizes around 10 nm is required to model lines of sight whose extinctions are similar to the average Galactic curve. We conclude that to be accurately described, the so-called peculiar extinction curves do not need dust grains with exotic properties. |
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| AbstractList | We investigate the remarkable variety of IR-through-UV extinction curves by modelling extinction profiles with core-mantle grains and a collection of single and stacked polycyclic aromatic hydrocarbons. Such a model can closely reproduce the observed curves, by simply assuming a different ratio of the molecular component to classical dust, while leaving relatively unmodified the underlying global picture. In particular, we find that for extinction curve morphologies differing significantly from the average Galactic extinction, dust grain sizes exhibit a low-end cut-off at approximately 100 nm. An additional component of very small grains of sizes around 10 nm is required to model lines of sight whose extinctions are similar to the average Galactic curve. We conclude that to be accurately described, the so-called peculiar extinction curves do not need dust grains with exotic properties. ABSTRACT We investigate the remarkable variety of IR‐through‐UV extinction curves by modelling extinction profiles with core‐mantle grains and a collection of single and stacked polycyclic aromatic hydrocarbons. Such a model can closely reproduce the observed curves, by simply assuming a different ratio of the molecular component to classical dust, while leaving relatively unmodified the underlying global picture. In particular, we find that for extinction curve morphologies differing significantly from the average Galactic extinction, dust grain sizes exhibit a low‐end cut‐off at approximately 100 nm. An additional component of very small grains of sizes around 10 nm is required to model lines of sight whose extinctions are similar to the average Galactic curve. We conclude that to be accurately described, the so‐called peculiar extinction curves do not need dust grains with exotic properties. ABSTRACT We investigate the remarkable variety of IR-through-UV extinction curves by modelling extinction profiles with core-mantle grains and a collection of single and stacked polycyclic aromatic hydrocarbons. Such a model can closely reproduce the observed curves, by simply assuming a different ratio of the molecular component to classical dust, while leaving relatively unmodified the underlying global picture. In particular, we find that for extinction curve morphologies differing significantly from the average Galactic extinction, dust grain sizes exhibit a low-end cut-off at approximately 100 nm. An additional component of very small grains of sizes around 10 nm is required to model lines of sight whose extinctions are similar to the average Galactic curve. We conclude that to be accurately described, the so-called peculiar extinction curves do not need dust grains with exotic properties. [PUBLICATION ABSTRACT] |
| Author | Zonca, A. Cecchi-Pestellini, C. Malloci, G. Mulas, G. |
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| Keywords | ultraviolet: ISM dust, extinction ISM: abundances Grain size Dust grain Polycyclic aromatic hydrocarbons Morphology Abundance Models Extinction curve |
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| Snippet | We investigate the remarkable variety of IR-through-UV extinction curves by modelling extinction profiles with core-mantle grains and a collection of single... ABSTRACT We investigate the remarkable variety of IR‐through‐UV extinction curves by modelling extinction profiles with core‐mantle grains and a collection of... ABSTRACT We investigate the remarkable variety of IR-through-UV extinction curves by modelling extinction profiles with core-mantle grains and a collection of... |
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| SubjectTerms | Astronomy dust dust, extinction Earth, ocean, space Exact sciences and technology extinction ISM: abundances Morphology Polycyclic aromatic hydrocarbons Star & galaxy formation ultraviolet: ISM |
| Title | Modelling peculiar extinction curves |
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