Field news
The astrophysical community is interested in collisions of species
with H, He, H2, e at collision energies up 500K and for internal
energy up to 1000K. Species that are of main interest are: C3, CH,
CH+, CCH, CH3CCH, CH3OCOH, CH3OH, CH2CHCN,
CH3CN, CH3CH2CN, CH3CH2OH, CN, CO, CCCS, CCS,
CS, H2CO, H3O+, H2O (vibrational), H2CS, H2S, HCl,
HCN, HCN (vibrational), HF, HC3N, HC5N, HCO, HCO+, HCOOH,
HNC, NH2, N2H+, NH3, SO, SO2, OCS, other prebiotic molecules.
Data on deuterated isotopes of the above molecules and especially
HDCO, HDCS, HDO, HDS are also necessary. For most of the above
systems, hyperfine transitions need to be taken into account. We also
need data for the following systems: H3+ + D2, HD + D2,
H2D+ + HD, H2D+ + D2, H2 + HD, H2 + D2,
D2H+ + D2, H2 + D2, HD + D2.