International audience(Abridged) We use HIFI maps of the 987 GHz H2O 2(02)-1(11) emission to measure the sizes and shapes of 19 high-mass protostellar envelopes. To identify infall, we use HIFI spectra of the optically thin C18O 9-8 and H2O-18 1(11)-0(00) lines. The high-J C18O line traces the warm central material and redshifted H2O-18 1(11)-0(00) absorption indicates material falling onto the warm core. We probe small-scale chemical differentiation by comparing H2O 752 and 987 GHz spectra with those of H2O-18. Our measured radii of the central part of the H2O 2(02)-1(11) emission are 30-40% larger than the predictions from spherical envelope models, and axis ratios are <2, which we consider good agreement. For 11 of the 19 sources, we fin...
International audience(Abridged) Water is a key tracer of dynamics and chemistry in low-mass protost...
International audienceWe derive the dense core structure and the water abundance in four massive sta...
Context. Water probes the dynamics in young stellar objects (YSOs) effectively, especially shocks in...
International audience(Abridged) We use HIFI maps of the 987 GHz H2O 2(02)-1(11) emission to measure...
Context. The physical conditions during high-mass star formation are poorly understood. Outflow and ...
Context. Water is a key constituent of star-forming matter, but the origin of its line emission and ...
Context. Water is a key constituent of star-forming matter, but the origin of its line emission and ...
International audienceTo understand the origin of water line emission and absorption during high-mas...
Context. Water is a key constituent of star-forming matter, but the origin of its line emission and ...
Context. Water is a key probe of shocks and outflows from young stars because it is extremely sensit...
Context. Water is an important chemical species in the process of star formation, and a sensitive tr...
International audience(Abridged) Water is a key tracer of dynamics and chemistry in low-mass protost...
International audienceWe derive the dense core structure and the water abundance in four massive sta...
Context. Water probes the dynamics in young stellar objects (YSOs) effectively, especially shocks in...
International audience(Abridged) We use HIFI maps of the 987 GHz H2O 2(02)-1(11) emission to measure...
Context. The physical conditions during high-mass star formation are poorly understood. Outflow and ...
Context. Water is a key constituent of star-forming matter, but the origin of its line emission and ...
Context. Water is a key constituent of star-forming matter, but the origin of its line emission and ...
International audienceTo understand the origin of water line emission and absorption during high-mas...
Context. Water is a key constituent of star-forming matter, but the origin of its line emission and ...
Context. Water is a key probe of shocks and outflows from young stars because it is extremely sensit...
Context. Water is an important chemical species in the process of star formation, and a sensitive tr...
International audience(Abridged) Water is a key tracer of dynamics and chemistry in low-mass protost...
International audienceWe derive the dense core structure and the water abundance in four massive sta...
Context. Water probes the dynamics in young stellar objects (YSOs) effectively, especially shocks in...