DustEM: Dust extinction and emission modelling

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kcd
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DustEM: Dust extinction and emission modelling

Post by kcd » Sat Jul 06, 2013 7:54 am

[c]DustEM: Dust extinction and emission modelling[/c][/b]
Abstract: DustEM computes the extinction and the emission of interstellar dust grains heated by photons. It is written in Fortran 95 and is jointly developed by IAS and CESR. The dust emission is calculated in the optically thin limit (no radiative transfer) and the default spectral range is 40 to 108 nm. The code is designed so dust properties can easily be changed and mixed and to allow for the inclusion of new grain physics.

Credit: Compiègne, M.; Verstraete, L.; Jones, A.; Bernard, J.-P.; Boulanger, F.; Flagey, N.; Le Bourlot, J.; Paradis, D.; Ysard, N.

Site: http://www.ias.u-psud.fr/DUSTEM/
http://adsabs.harvard.edu/abs/2011A%26A...525A.103C

Bibcode: 2013ascl.soft07001C

Preferred citation method: http://adsabs.harvard.edu/abs/2011A%26A...525A.103C

ID: ascl:1307.001
Last edited by Ada Coda on Sun Aug 19, 2018 9:43 am, edited 1 time in total.
Reason: Updated code entry.

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