Organic Matter in Space - an Overview
arXiv:0807.0857 · doi:10.1017/S1743921308021078
Abstract
Organic compounds are ubiquitous in space: they are found in diffuse clouds, in the envelopes of evolved stars, in dense star-forming regions, in protoplanetary disks, in comets, on the surfaces of minor planets, and in meteorites and interplanetary dust particles. This brief overview summarizes the observational evidence for the types of organics found in these regions, with emphasis on recent developments. The Stardust sample-return mission provides the first opportunity to study primitive cometary material with sophisticated equipment on Earth. Similarities and differences between the types of compounds in different regions are discussed in the context of the processes that can modify them. The importance of laboratory astrophysics is emphasized.
Introductory overview lecture presented at IAU Symposium 251, "Organic matter in space", held at Hong Kong, February 2008; to appear in IAU Symposium 251 proceedings, Cambridge University Press, ed. S. Kwok et al
References in corpus (9)
- Testing grain-surface chemistry in massive hot-core regions
- Discovery of Interstellar Propylene (CH_2CHCH_3): Missing Links in Interstellar Gas-Phase Chemistry
- Spatially extended PAHs in circumstellar disks around T Tauri and Herbig Ae stars
- PAH chemistry and IR emission from circumstellar disks
- Complex Organic Materials in the Circumstellar Disk of HR 4796A
- H-atom bombardment of CO2, HCOOH and CH3CHO containing ices
- Spatial separation of small and large grains in the transitional disk around the young star IRS 48
- Photodissociation of small carbonaceous molecules of astrophysical interest
- Carbonates in space - The challenge of low temperature data