“…In these environments charge transfer plays an important role. Recent studies of ionmolecule charge transfer include He 2+ (Dubois et al 2005, Kusakabe et al 2006, C 4+ (Zarour et al 2005), O + , O 5+ and Ar 5+ (Dubois et al 2005), and F 7+ (Zouros et al 2008) with H 2 ; H + (Lindsay et al 2005a, Wells et al 2005, Kumar et al 2006, Lin et al 2007 and He 2+ (Kusakabe et al 2006) , He 2+ (Bodewits, et al 2005, Seredyuk et al 2005c, O 6+ (Seredyuk et al 2005b, Bodewits & Hoekstra 2007, and a range of ions (Otranto & Olson 2008) (Seredyuk et al 2005a), and C 4+ and O 6+ (Seredyuk et al 2005b) with CH 4 ; H + (Suzuki et al 2005) and He 2+ (Seredyuk et al 2005a) with C 2 H 4 ; and He 2+ (Seredyuk et al 2005a) For applications to x-ray emission from comets and planetary atmospheres, charge exchange has been considered for molecular targets including C (3−6)+ , N (4−7)+ , and O (5−7)+ with methane (Djurić et al 2008); highly charged L-shell Fe ions with various neutrals (Wargelin et al 2005, Beiersdorfer et al 2008; and for a range of ions and molecules (Otranto et al 2006). …”