H2 – Commission H2 Astrochemistry
Description
Commission H2 Astrochemistry is an upgrade of a long-running and successful Working Group of the same name. The topic reflects one of growing importance within astronomy – the use of molecular emission and absorption lines to probe objects as diverse as planetary atmospheres and comets within our Solar System to distant galaxies at redshift greater than 6. In addition to the intrinsic value of studying astrochemistry to astronomy, there is an additional benefit to chemistry in that conditions in the interstellar medium are so extreme in terms of temperature, densities, size and time scales not easily accessible to terrestrial laboratories. Thus astrochemistry attracts scientists from a number of different disciplines such as chemistry and planetary science. It directly connects with new fields such as astrobiology and the study of exoplanets and their atmospheres. Because of this broad perspective, astrochemistry is a rich and vibrant field and the purpose of the Commission is to promote such connections.
Under Division
Division H Interstellar Matter and Local Universe
Commission Working Groups
Inter-Commission C1-F2-F3-H2 WG Education and Training in Astrobiology
University of Copenhagen
Niels Bohr Institute
Oester Voldgade 5-7
1350 K Copenhagen
Denmark
Phone: +45 35324186
Personal website: http://youngstars.nbi.dk
Organization website: http://www.nbi.dk
NCA adherence: Denmark
Last updated:
November 20, 2023
MPIA
Planet- and Star-Formation
Koenigstuhl 17
69117 Heidelberg
Germany
Phone: +49 06221528354
Organization website: http://www.mpia.de/homes/semenov
NCA adherence: Germany
Last updated:
October 21, 2024
Organizing Committee