Abstract.
The Herschel Space Observatory has been revolutionizing our
understanding of the the earliest phases of star formation. In this
contribution, we describe early results from the Gould Belt Survey,
a Herschel Key Project to map 15 nearby molecular clouds in
continuum emission from 70 μm to 500 μm.
In particular, I describe how the sensitive and wide maps of the
Aquila Rift have strongly confirmed the similarity between the shapes
of the stellar Initial Mass Function and the prestellar core mass
function
(CMF). Also, the Herschel map sensitivity to larger scale
emission
has revealed
that prestellar cores form almost exclusively within dense filaments
that exceed a critical mass per unit length defined by temperature (and
gravity). Finally, filaments in three clouds, IC 5146, Polaris and
Aquila,
are found to have similar widths of ∼0.1 pc, approximately the
scale where the turbulent velocity equals the sound speed of 10 K gas.
This
common width suggests filaments themselves are formed through
collisional
shocks of turbulent flows and evolve in quasi-virial balance
through mass accretion.
Key words:far-infrared/submillimetre -- prestellar cores --
Herschel Space Observatory