The 2014 KIDA Network for Interstellar Chemistry

• Chemical models used to study the chemical composition of the gas and the ices in the interstellar medium are based on a network of chemical reactions and associated rate coefficients. These reactions and rate coefficients are partially compiled from data in the literature, when available. We present in this paper kida.uva.2014, a new updated version of the kida.uva public gas-phase network first released in 2012. In addition to a description of the many specific updates, we illustrate changes in the predicted abundances of molecules for cold dense cloud conditions as compared with the results of the previous version of our network, kida.uva.2011.

Ämnesord

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)

NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Nyckelord

astrochemistry

astronomical databases: miscellaneous

ISM: abundances

ISM: molecules

astrochemistry

astronomical databases: miscellaneous

ISM: abundances

ISM: molecules

Publikations- och innehållstyp

ref (ämneskategori)

art (ämneskategori)