TY - JOUR
T1 - TRANSLATIONAL AND ROTATIONAL ENERGY MEASUREMENTS OF PHOTODESORBED WATER MOLECULES IN THEIR VIBRATIONAL GROUND STATE FROM AMORPHOUS SOLID WATER
AU - Yabushita, Akihiro
AU - Hama, Tetsuya
AU - Yokoyama, Masaaki
AU - Kawasaki, Masahiro
AU - Andersson, Stefan
AU - Dixon, Richard N.
AU - Ashfold, Michael N. R.
AU - Watanabe, Naoki
PY - 2009/7/10
Y1 - 2009/7/10
N2 - For interstellar grains coated with water ice, the most important desorption mechanism at the edge of molecular clouds is photodesorption of water. To reveal details of the photodesorption mechanism, we have measured the translational and rotational energies of H2O (v = 0) molecules photodesorbed from amorphous solid water and polycrystalline ice following excitation within the first absorption band using a 157 nm laser. The measured translational and rotational temperatures are 1800 K and 300 K, respectively. These energies are in good accord with those predicted by classical molecular dynamics calculations for the "kick-out" of an H2O molecule in the ice by an energetic H atom. The statistical ortho: para ratio of g(OPR) = 3 is appropriate for the Boltzmann rotational distribution of the H2O molecules.
AB - For interstellar grains coated with water ice, the most important desorption mechanism at the edge of molecular clouds is photodesorption of water. To reveal details of the photodesorption mechanism, we have measured the translational and rotational energies of H2O (v = 0) molecules photodesorbed from amorphous solid water and polycrystalline ice following excitation within the first absorption band using a 157 nm laser. The measured translational and rotational temperatures are 1800 K and 300 K, respectively. These energies are in good accord with those predicted by classical molecular dynamics calculations for the "kick-out" of an H2O molecule in the ice by an energetic H atom. The statistical ortho: para ratio of g(OPR) = 3 is appropriate for the Boltzmann rotational distribution of the H2O molecules.
U2 - 10.1088/0004-637X/699/2/L80
DO - 10.1088/0004-637X/699/2/L80
M3 - Article (Academic Journal)
SN - 1538-4357
VL - 699
SP - L80-L83
JO - Astrophysical Journal
JF - Astrophysical Journal
IS - 2
ER -