The Formation of Complex Organic Molecules in Star-Forming Regions

Presenter: Eric Herbst, University of Virginia
When: March 10, 2014 11AM PDT

A large number of organic molecules have been detected in the gas phase of interstellar clouds. Interestingly, the molecules found in very cold clouds (10 K) with little star formation are exotic by terrestrial standards while the molecules found in regions of star and planet formation tend to be more terrestrial in nature. The synthesis of the exotic molecules is ironically well understood in terms of gas- phase ion-molecule reactions, which tend to produce very unsaturated species, as well as ions, both positively and negatively charged, isomers, and radicals. On the other hand, the formation of more hydrogen-rich terrestrial-type organic molecules in star-forming regions is not well understood.

Most investigators feel, however, that reactions on interstellar dust particles followed by sublimation into the gas as temperatures rise play a major role. In my talk, I will discuss current models of how complex molecules are formed in several evolutionary stages of star formation including so-called hot cores and corinos as well as protoplanetary disks.

NAI Director's Seminar Series

  • The Director’s Seminar series features talks from scientists who are invited by the NAI Director to present their research results to the community. A primary goal of the seminars is to encourage interdisciplinary collaboration across NAI teams and within the astrobiology community at large.
  • Subscribe to this series

Other Seminars in this Series