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20072026
most citedThe UMIST database for astrochemistry 2012

991 citations · 4.6k across the 118 of their papers we have counts for

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astro-ph.SR2012★ 991 cited

The UMIST database for astrochemistry 2012

D. McElroy, C. Walsh, A. J. Markwick +3

We present the fifth release of the UMIST Database for Astrochemistry (UDfA). The new reaction network contains 6173 gas-phase reactions, involving 467 species, 47 of which are new…

astro-ph.GA2012★ 28 cited

Small-scale structure in the interstellar medium: time-varying interstellar absorption towards κ Velorum

Keith T. Smith, Stephen J. Fossey, Martin A. Cordiner +4

Ultra-high spectral resolution observations of time-varying interstellar absorption towards κ Vel are reported, using the Ultra-High Resolution Facility on the Anglo-Australian Tel…

astro-ph.SR2012★ 78 cited

Isotopic Anomalies in Primitive Solar System Matter: Spin-state Dependent Fractionation of Nitrogen and Deuterium in Interstellar Clouds

E. S. Wirström, S. B. Charnley, M. A. Cordiner +1

Organic material found in meteorites and interplanetary dust particles is enriched in D and 15N. This is consistent with the idea that the functional groups carrying these isotopic…

astro-ph.GA2012★ 12 cited

The chemistry of extragalactic carbon stars

Paul M. Woods, Catherine Walsh, Martin A. Cordiner +1

Prompted by the ongoing interest in Spitzer Infrared Spectrometer spectra of carbon stars in the Large Magellanic Cloud, we have investigated the circumstellar chemistry of carbon…

astro-ph.GA2012★ 56 cited

The abundance of C3H2 and other small hydrocarbons in the diffuse interstellar medium

Harvey Liszt, Paule Sonnentrucker, Martin Cordiner +1

Hydrocarbons are ubiquitous in the interstellar medium, observed in diverse environments ranging from diffuse to molecular dark clouds and strong photon-dominated regions near HII…

astro-ph.GA2012★ 28 cited

Gas-grain models for interstellar anion chemistry

M. A. Cordiner, S. B Charnley

Long-chain hydrocarbon anions CnH- (n=4, 6, 8) have recently been found to be abundant in a variety of interstellar clouds. In order to explain their large abundances in the denser…