Dissociative recombination is a corner-stone reaction in the synthesis of interstellar molecules and plays an important role in the ionised layers of the atmospheres of the Earth, other planets, and their satellites. The studies of dissociative recombination reactions was for a long time dominated by afterglow techniques, and these techniques are used in improved versions also today, but the bulk of the relevant data have in recent years been produced at ion storage rings. We review briefly these different experimental techniques. As examples of recent developments in the field, we discuss in particular the dissociative recombination of H 3 + , the role of dissociative recombination in the chemistry of hydrocarbons and sulphur compounds in the interstellar medium and planetary ionospheres, and the synthesis of interstellar methanol.
Keywords: Dissociative Recombination, Ion-electron interaction, interstellar medium, planetary ionospheres
AMS Subject Classification: 85-05
IntroductionHalf a century ago, when this journal was founded, interstellar clouds were thought to be essentially atomic with a small component of diatomic molecules. Now the situation is radically different. The realization that the Universe is highly molecular has led to new areas of astronomy such as astrochemistry and molecular astrophysics. Prestigious conferences, such as several Faraday Discussions [1,2], International Astronomical Union meetings [3, 4, 5, 6, 7, 8], and the Nobel Symposium No 133 [9] have been devoted to these new areas. Astrochemistry was also a theme in the 5 th International Chemical Congress of Pacific Basin Societies (PACIFICHEM) [10] and a special feature issue on the subject has been published in the Proceedings of the National Academy of Sciences [11]. Molecules are ubiquitous almost anywhere in the Universe cooler than sunspots.Dissociative recombination (DR) of molecular ions with electrons was first discussed in connection with the Earth's ionosphere, with photoionisation being the source of free electrons and DR the sink [12]. When synthetic schemes based on ion-molecule reactions were introduced to explain molecular abundances [13, 14], they scored an immediate success with the prediction of HCO + [15] as the carrier of the interstellar 89.190 GHz line [16], later confirmed by laboratory molecular spectroscopy [17], dissociative recombination became an important part of the scheme for interstellar molecule formation. In this article we 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36 37 38 39 40 41 42 43 44 45 46 47 48 49 50 51 52 53 54 55 56 57 58 59 Recent reviews of dissociative recombination have been written by , Adams, Poterya and Babcock [19], and Thomas [20], and a research monograph by Larsson and Orel [21] has just been published. It would by far exceed the scope of this article to cover all dissociative recombination processes that are relevant in the interstellar medium and p...