Rotational excitation of 45 levels of ortho/para-H2O by excited ortho/para-H2from 5 K to 1500 K: state-to-state, effective, and thermalized rate coefficients

Water in Star-forming Regions with theHerschel Space Observatory(WISH). I. Overview of Key Program and First Results

(2011) E. F. van Dishoeck et al.   PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC

Water in low-mass star-forming regions withHerschel

(2010) L. E. Kristensen et al.   ASTRONOMY & ASTROPHYSICS

Variations in H2O+/H2O ratios toward massive star-forming regions

(2010) F. Wyrowski et al.   ASTRONOMY & ASTROPHYSICS

Water in massive star-forming regions: HIFI observations of W3 IRS5

(2010) L. Chavarría et al.   ASTRONOMY & ASTROPHYSICS

Rotational excitation of 20 levels of para-H2O by ortho-H2(j2= 1, 3, 5, 7) at high temperature

(2010) F. Daniel et al.   ASTRONOMY & ASTROPHYSICS

Water abundances in high-mass protostellar envelopes:Herschelobservations with HIFI

(2010) M. G. Marseille et al.   ASTRONOMY & ASTROPHYSICS

Sensitive limits on the abundance of cold water vapor in the DM Tauri protoplanetary disk

(2010) E. A. Bergin et al.   ASTRONOMY & ASTROPHYSICS

Warm water vapour in the sooty outflow from a luminous carbon star

(2010) L. Decin et al.   NATURE

Rotational excitation of ortho-H2O by para-H2 (j2 = 0, 2, 4, 6, 8) at high temperature

(2009) M.-L. Dubernet et al.   ASTRONOMY & ASTROPHYSICS

R12-calibrated H2O–H2 interaction: Full dimensional and vibrationally averaged potential energy surfaces

(2008) Pierre Valiron et al.   JOURNAL OF CHEMICAL PHYSICS