Gas and Dust in the Orion Bar

Details Gas and Dust in the Orion Bar Gas and Dust in the Orion Bar

Nov 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011eas....52..277a&link_type=abstract

EAS Publications Series, Volume 52, 2011, pp.277-279

Physics

Scientific paper

We use the DustEM model coupled with a radiative transfer code to fit the Herschel and Spitzer emission of the Orion Bar. The thermal dust emission at the 250-μm peak position is well reproduced but we overestimate the stochastically heated grain emission. The dust model parameters are checked with the Meudon PDR code and are consistent with the spectroscopic data from the SPIRE FTS.

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