Christopher M. Wright

Herschel/PACS spectroscopy of NGC 4418 and Arp 220: H₂O, H₂¹⁸O, OH,¹⁸OH, O I, HCN, and NH₃

The Mrk 231 molecular outflow as seen in OH

The far-infrared emitting region in local galaxies and QSOs: Size and scaling relations

UV Circular Polarisation in Star Formation Regions: The Origin of Homochirality?

An astrophysically-relevant mechanism for amino acid enantiomer enrichment

Heterocyclic Carbenes: Synthesis and Coordination Chemistry

Experimental Investigation on the Formation of Carbon-Bearing Molecules in the Interstellar Medium via Neutral−Neutral Reactions

The determination of the void structure of microporous coals by small-angle neutron scattering: Void geometry and structure in Illinois No. 6 bituminous coal

eCommerce: a critical review

The Galactic Center massive black hole and nuclear star cluster

Investigating Disk Evolution: A High Spatial Resolution Mid‐Infrared Survey of T Tauri Stars

Essentials ofk-essence

Characterization of gas shale pore systems by porosimetry, pycnometry, surface area, and field emission scanning electron microscopy/transmission electron microscopy image analyses: Examples from the Barnett, Woodford, Haynesville, Marcellus, and Doig units

The importance of shale composition and pore structure upon gas storage potential of shale gas reservoirs

Using Laboratory Spectroscopy to Identify Lines in theK‐ andL‐Band Spectrum of Water in a Sunspot

Variation in micropore capacity and size distribution with composition in bituminous coal of the Western Canadian Sedimentary Basin

Primordial nucleosynthesis: theory and observations

HITEMP, the high-temperature molecular spectroscopic database

Coalbed methane: A review

A new collection of real world applications of fractional calculus in science and engineering

Information systems in supply chain integration and management

The Water Vapor Abundance in Circumstellar Envelopes

The many lives of active galactic nuclei: Cooling flows, black holes and the luminosities and colours of galaxies

SHINING, A Survey of Far-infrared Lines in Nearby Galaxies. I. Survey Description, Observational Trends, and Line Diagnostics

The Excitation and Metallicity of Galactic HiiRegions fromInfrared Space ObservatorySWS Observations of Mid‐Infrared Fine‐Structure Lines

AGN feedback in a galaxy merger: Multi-phase, galaxy-scale outflows with a fast molecular gas blob ~6 kpc away from IRAS F08572+3915

CBM and CO2-ECBM related sorption processes in coal: A review

Silicate Emission in T Tauri Stars: Evidence for Disk Atmospheres?

Moisture in coal

First‐Year Wilkinson Microwave Anisotropy Probe ( WMAP ) Observations: Determination of Cosmological Parameters

The evolution and explosion of massive stars

Gas Diffusion in Fractal Porous Media

Pore structure characterization of North American shale gas reservoirs using USANS/SANS, gas adsorption, and mercury intrusion

Coal physical structure: porous rock and macromolecular network

Spatial Variability in the Ratio of Interstellar Atomic Deuterium to Hydrogen. I. Observations toward δ Orionis by the Interstellar Medium Absorption Profile Spectrograph

Clean liquid fuels from direct coal liquefaction: chemistry, catalysis, technological status and challenges

Spatial Variability in the Ratio of Interstellar Atomic Deuterium to Hydrogen. II. Observations toward γ²Velorum and ζ Puppis by the Interstellar Medium Absorption Profile Spectrograph

DIAGNOSTICS OF AGN-DRIVEN MOLECULAR OUTFLOWS IN ULIRGs FROMHERSCHEL-PACS OBSERVATIONS OF OH AT 119 μm

No Fossil Disk in the T Tauri Multiple System V773 Tauri

Imagineering the Future of the Internet: Sketches from the Year 2010

Detection of HD in the Orion molecular outflow

Mid-infrared spectropolarimetry of molecular cloud sources : magnetic fields and dust properties

[ITAL]Infrared Space Observatory[/ITAL]–Long Wavelength Spectrometer Detection of the 112 Micron HD [ITAL]J[/ITAL] = 1 → 0 Line toward the Orion Bar

Application of small-angle neutron scattering (SANS) to the study of coal porosity

Radiative Transfer Models of Emission and Absorption in the H[TINF]2[/TINF]O 6 Micron Vibration-Rotation Band toward Orion-BN-KL

The [ITAL]ISO[/ITAL]–SWS 2.4–45.2 Micron Spectrum toward Orion IR[CLC]c[/CLC]2