H O CO and CO / Aeronautics Administration / CGAS / Product CO / Gasphase CO / Bernstein / /
Country
United States / /
Currency
pence / /
Facility
Kuiper Airborne Observatory / University of Hawaii / Infrared Telescope Facility / SETI Institute / Kapteyn Astronomical Institute / Infrared Space Observatory / NASA Infrared Telescope Facility / /
IndustryTerm
lowest energy level / high-energy protons / gas-phase lines / carbon-nitrogen carrier / Energetic processing / high-energy ions / interstellar gas / gas phase al. / planetary systems / gas phase / energy / /
MusicGroup
ISM / È / N / UV / /
NaturalFeature
Mauna Kea / /
Organization
University of Hawaii / Internal Revenue Service / NASA Ames Research Center / SETI Institute / National Aeronautics and Space Administration / Kapteyn Astronomical Institute / American Astronomical Society / National Space and Aeronautics Administration / Institute for Astronomy / /
Person
Cristina Dalle Ore / Jean Chiar / Elisabetta Palumbo / Karin Demyk / van IJzendoorn / Jacqueline Keane / Steve Charnley / Infrared Telescope / /
Position
Visiting Astronomer / /
Product
Cooled Grating Array Spectrometer / /
ProvinceOrState
Alabama / New Foundland and Labrador / Hawaii / California / Colorado / New Hampshire / /
THE ASTROPHYSICAL JOURNAL, 513 : 294È304, 1999 March[removed]The American Astronomical Society. All rights reserved. Printed in U.S.A. THE INTERSTELLAR 4.62 MICRON BAND Y. J. PENDLETON,1 A. G. G. M. TIELENS,2,3 A. T.