Characterising the high-mass star forming filament G351.776--0.527 with Herschel and APEX dust continuum and gas observations

S. Leurini, E. Schisano, T. Pillai +13

G351.776-0.527 is among the most massive, closest, and youngest filaments in the inner Galactic plane and therefore it is an ideal laboratory to study the kinematics of dense gas a…