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CHEMICAL EVOLUTION OF PROTOSTELLAR MATTER WILLIAM D. LANGER Jet Propulsion Laboratory EWINE F. VAN DISHOECK Leiden Observatory EDWIN A. BERGIN
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Document Date: 2007-04-05 13:30:16


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Flux (Jy) CO2 1 10 CO / O and CO / Solid CO / McCall / THANGASAMY VELUSAMY Jet Propulsion Laboratory / Suzuki / /

Facility

Technology ALEXANDER G. G. M. TIELENS Kapteyn Astronomical Institute THANGASAMY VELUSAMY Jet Propulsion Laboratory / Infrared Space Observatory / /

IndustryTerm

thermal processing / kinetic gas temperature / clumped gas / gas-phase / chemical evolution / chemical composition / carbon chain / grain-dependent chemical processing / chemical processes / interstellar and circumstellar gas / chemical gradients / ion-molecule chemistry networks / chemical evolutionary models / chemical differentiation / Gas-grain interactions / interstellar gas / lowtemperature gas-phase reactions / gas-phase molecules / planetary systems / protosolar systems / chemical studies / gas phase / warm/hot gas / /

MusicGroup

Interstellar / /

Organization

California Institute of Technology / African Union / Rensselaer Polytechnic Institute / Infrared Space Observatory Short Wavelength Spectrometer / Smithsonian / /

Person

Mundy / F. VAN DISHOECK / EDWIN A. BERGIN / GEOFFREY A. BLAKE / WILLIAM D. LANGER / van Dishoeck / DOUGLAS C. B. WHITTET / /

Position

player / /

ProvinceOrState

Alabama / Colorado / /

Technology

radiation / sublimation / AV / /

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