Sandford S. A. / Downs Laboratory / Bernstein / L. J. & Sandford S. A. / XCN AND CO / Cox / /
Country
Germany / Netherlands / France / United Kingdom / /
Event
Man-Made Disaster / /
Facility
Mauna Kea Observatory / Downs Laboratory of Physics / Rensselaer Polytechnic Institute / SETI Institute / California Institute of Technology / Infrared Space Observatory / /
IndustryTerm
chemical evolution / hot gas-phase chemistry / carrier species / hot gas / thermal processing / energy source / ubiquitous products / Gas-phase reactions involving species / gas-phase hydrogen column density / gas-phase cyanate abundances / nitrogen carrier / interstellar gas / gas phase / gas-phase nitrile concentrations / energetic processing tion / /
MusicGroup
ISM / È / /
OperatingSystem
Cygnus / /
Organization
California Institute of Technology / Internal Revenue Service / SETI Institute / ISAS / Department of Physics / Applied Physics and Astronomy / New York Center for Studies / Rensselaer Polytechnic Institute / NASA Ames Research Center / National Aeronautics and Space Administration / American Astronomical Society / /
Person
Biosphere / McLean / ESA SP / /
Position
D. J. / /
Product
Cyg OB2 / /
ProvinceOrState
Alabama / Hawaii / New York / South Carolina / California / Colorado / New Hampshire / /
THE ASTROPHYSICAL JOURNAL, 550 : 793È798, 2001 April[removed]The American Astronomical Society. All rights reserved. Printed in U.S.A. OBSERVATIONAL CONSTRAINTS ON THE ABUNDANCE AND EVOLUTION OF ““ XCN ÏÏ IN INT