Interstellar water chemistry: from laboratory to observations

EF Van Dishoeck, E Herbst, DA Neufeld - Chemical Reviews, 2013 - ACS Publications
Water is a fundamental molecule in the universe. On Earth, water exists in all three phases:
gas, liquid, and solid (ice). Liquid water facilitates many chemical reactions as a solvent …

Surface processes on interstellar amorphous solid water: Adsorption, diffusion, tunneling reactions, and nuclear-spin conversion

T Hama, N Watanabe - Chemical reviews, 2013 - ACS Publications
Since we intend to review experimental and theoretical studies of physicochemical
processes occurring on cosmic dust grains in very cold regions in space, we start with a brief …

Water in star-forming regions: physics and chemistry from clouds to disks as probed by Herschel spectroscopy

EF van Dishoeck, LE Kristensen, JC Mottram… - Astronomy & …, 2021 - aanda.org
Context. Water is a key molecule in the physics and chemistry of star and planet formation,
but it is difficult to observe from Earth. The Herschel Space Observatory provided …

A general model for the CO–H2 conversion factor in galaxies with applications to the star formation law

D Narayanan, MR Krumholz, EC Ostriker… - Monthly Notices of …, 2012 - academic.oup.com
The most common means of converting an observed CO line intensity into a molecular gas
mass requires the use of a conversion factor (X CO). While in the Milky Way this quantity …

Chemical evolution of star-forming regions

EF Van Dishoeck, GA Blake - Annual Review of Astronomy and …, 1998 - annualreviews.org
▪ Abstract Recent advances in the understanding of the chemical processes that occur
during all stages of the formation of stars, from the collapse of molecular clouds to the …

Chemistry of dark clouds: databases, networks, and models

M Agúndez, V Wakelam - Chemical Reviews, 2013 - ACS Publications
The introduction of chemistry into astronomy is relatively recent and can be dated back to
about half a century ago, when molecules were discovered in space. In the 1930s it was …

[图书][B] Dust in the galactic environment

DCB Whittet - 2018 - taylorfrancis.com
Dust is a ubiquitous feature of the cosmos, impinging directly or indirectly on most fields of
modern astronomy and astrophysics. Dust in the Galactic Environment, Second Edition …

The ionization fraction in dense cloud cores

P Caselli, CM Walmsley, R Terzieva… - The Astrophysical …, 1998 - iopscience.iop.org
The degree of ionization, x (e)= n (e)/n (H 2), and the cosmic-ray ionization rate, ζ, in 24
cloud cores have been determined by comparing observational data from Butner et al. on …

Molecular ions in L1544. II. The ionization degree

P Caselli, CM Walmsley, A Zucconi… - The Astrophysical …, 2002 - iopscience.iop.org
The maps presented in Paper I are here used to infer the variation of the column densities of
HCO+, DCO+, N 2 H+, and N 2 D+ as a function of distance from the dust peak. These …

Ion chemistry in space

M Larsson, WD Geppert, G Nyman - Reports on Progress in …, 2012 - iopscience.iop.org
We review the gas-phase chemistry in extraterrestrial space that is driven by reactions with
atomic and molecular ions. Ions are ubiquitous in space and are potentially responsible for …