ATLASGAL -- A Galaxy-wide sample of dense filamentary structures
  [Abridged] Aims. We study the properties of filamentary structures from the
ATLASGAL survey.
  Methods. We use the DisPerSE algorithm to identify spatially coherent
structures located across the inner-Galaxy (300 < l < 60 and |b| < 1.5).
  Results. We have determined distances, masses and physical sizes for 241 of
the filamentary structures. We find a median distance of 3.8 kpc, a mean mass
of a few 10^3 m_sun, a mean length of ~6pc and a mass-to-length ratio of (M/L)
~200-2000M_sun/ pc. We also find that these filamentary structures are tightly
correlated with the spiral arms in longitude and velocity, and that their
semi-major axis is preferentially aligned parallel to the Galactic mid-plane
and therefore with the direction of large-scale Galactic magnetic field. We
find many examples where the dense filaments identified in ATLASGAL are
associated with larger scale filamentary structures (~100 pc), and argue that
this is likely to be common, and as such these may indicate a connection
between large-scale Galactic dynamics and star formation.
  Conclusions. We have produced a large and Galaxy-wide catalogue of dense
filamentary structures that are representative of a particular size and mass
range not previously well studied in the literature. Analyses of the properties
and distribution of these filaments reveals that they are correlated with the
spiral arms and make a significant contribution to star formation in the
Galaxy. Massive star formation is ongoing within ~20% of the filaments and is
strongly correlated with the filaments with the largest mass-to- length ratios.
The luminosity of the embedded sources has a similar distribution to the
Galactic-wide samples of young massive stars and can therefore be considered to
be representative.
