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Laboratory astrochemistry at infrared wavelengths and molecular structure

Applicant Dr. Sven Thorwirth
Subject Area Astrophysics and Astronomy
Term from 2009 to 2018
Project identifier Deutsche Forschungsgemeinschaft (DFG) - Project number 88839181
 
Final Report Year 2017

Final Report Abstract

Fortunately, quite a few of the original ideas have turned into reality over the funding period to “pay my debts”, for example, the isotopic spectroscopy of carbon rich clusters (C3 , SiC3 Si, C3 S, SC3 S), the high resolution spectroscopy of Si2 C finally culminating in its astronomical detection, the high-resolution infrared study of GeC3 Ge and the spectroscopic detection of several carbon-sulfur chains as long as SC7 S by similar techniques. An astronomical detection of Si2 C could not be expected at the beginning but its discovery during was very exciting indeed! In IRC+10216, Si2 C is found to be very abundant and to play a key role in the formation of silicon-carbon dust grains. The laboratory infrared detection of a cluster as complex as SC7 S was kind of a surprise but is a clear manifestation of the possibilities provided by high-resolution infrared spectroscopy of a free jet. For sure, other binary carbon-rich chain systems involving even more exotic elements than S and Si, are very interesting future targets. As we have shown through our study of GeCCCGe for example, high-resolution infrared spectroscopy can provide very important structural information for carbon-rich systems. Still, for many such fundamental systems virtually no spectroscopic and structural information is known from experiment. As we have shown at a later stage of the funding period, new areas like carbon clusters ions are very promising fields of research to be entered in the future. A first step into this direction was already successfully taken as shown through the detection of C3 + and HC3 O+ , studies that offer many more future possibilities. The collaboration with Dr. Michael C. McCarthy at Harvard University has permitted the detection of many highly interesting transient molecules. This branch of research performed here offers possibilities for subsequent radio astronomical searches. Many of the molecules are found to exhibit very interesting/exotic molecular structures and might even be considered as textbook examples for structural chemistry.

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