Far-infrared emission from dust in the BOK globule Barnard 335

Details Far-infrared emission from dust in the BOK globule Barnard 335 Far-infrared emission from dust in the BOK globule Barnard 335

Jun 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993mnras.262..805d&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 262, no. 3, p. 805-811.

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2

Cosmic Dust, Emission Spectra, Far Infrared Radiation, Astronomical Models, Radiation Distribution, Radiative Transfer, Star Formation, Thermal Emission

Scientific paper

By using a detailed radiative transfer model, we show that the observed FIR spectrum of the Bok globule Barnard 335 can be explained by dust emission whose only energy source is the interstellar radiation field. The anomalous excess radiation observed around 60 microns in B335 and other globules can be accounted for by a 'nonconventional' dust component, the very small grains already proposed for other celestial objects.

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