Interstellar dust in the BOOMERanG maps

Details Interstellar dust in the BOOMERanG maps Interstellar dust in the BOOMERanG maps

May 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aipc..616...18m&link_type=abstract

EXPERIMENTAL COSMOLOGY AT MILLIMETRE WAVELENGTHS: 2K1BC Workshop. Breuil-Cervinia, Valle d'Aosta, Italy, 9-13 July, 2001. Edit

Computer Science

Databases

3

Radio, Microwave, Interstellar Dust Grains, Diffuse Emission, Infrared Cirrus, Background Radiations, Astronomical Catalogs, Atlases, Sky Surveys, Databases, Retrieval Systems, Archives, Etc.

Scientific paper

Interstellar dust (ISD) emission is present in the mm-wave maps obtained by the BOOMERanG experiment at intermediate and high Galactic latitudes. We find that, while being sub-dominant at the lower frequencies (90, 150, 240 GHz), thermal emission from ISD is dominant at 410 GHz, and is well correlated with the IRAS map at 100 μm. We find also that the angular power spectrum of ISD fluctuations at 410 GHz is a power law, and its level is negligible with respect to the angular power spectrum of the Cosmic Microwave Background (CMB) at 90 and 150 GHz. .

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