Interstellar H(3)(+).
Protonated molecular hydrogen, H(3)(+), is the simplest polyatomic molecule. It is the most abundantly produced interstellar molecule, next only to H(2), although its steady state concentration is low because of its extremely high chemical reactivity. H(3)(+) is a strong acid (proton donor) and initiates chains of ion-molecule reactions in interstellar space thus leading to formation of complex molecules. Here, I summarize the understandings on this fundamental species in interstellar space obtained from our infrared observations since its discovery in 1996 and discuss the recent observations and analyses of H(3)(+) in the Central Molecular Zone near the Galatic center that led to a revelation of a vast amount of warm and diffuse gas existing in the region.
Oka
Takeshi
T
Departments of Chemistry and Astronomy and Astrophysics, Enrico Fermi Institute, University of Chicago, Chicago, IL 60637, USA. t-oka@uchicago.edu
D001256:Astronomy / Q000295:instrumentation / Q000379:methods; D019443:Cosmic Dust; D005118:Extraterrestrial Environment / Q000737:chemistry*; D006859:Hydrogen / Q000737:chemistry*
D019443:Cosmic Dust; D006859:Hydrogen