Distribution of the Thermal Dust Temperature and Optical Depth in the Solar Neighborhood, Searching for the Dark Molecular Gas Component

Details Distribution of the Thermal Dust Temperature and Optical Depth in the Solar Neighborhood, Searching for the Dark Molecular Gas Component Distribution of the Thermal Dust Temperature and Optical Depth in the Solar Neighborhood, Searching for the Dark Molecular Gas Component

Jan 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aas...21724321p&link_type=abstract

American Astronomical Society, AAS Meeting #217, #243.21; Bulletin of the American Astronomical Society, Vol. 43, 2011

Astronomy and Astrophysics

Astronomy

Scientific paper

Using Planck maps combined with IRAS data, we construct all-sky maps of
the dust apparent temperature and optical depth. The optical depth maps
are used to look for excess emission with respect to neutral and
molecular gas tracers in order to investigate the presence of dark
molecular gas and to quantify its importance in the solar neighborhood.

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