San Francisco / Cambridge / Ashok / Lyon / Mount Wilson / TUTHILL ET / /
Company
Hale D. D. / Stellar Systems / Space Sciences Laboratory / /
Country
United States / Australia / /
Facility
Smithsonian Astrophysical Observatory / California Institute of Technology / Infrared Space Observatory / University of California / University of Sydney / W. M. Keck Observatory / /
IndustryTerm
spectral energy distribution / spectral energy distributions / broadband spectral energy distribution / high angular resolution imaging / similar spectral energy distributions / data processing techniques / synthetic spectral energy distributions / separated-element imaging interferometers / density-radius law / imaging / energy distribution / simulated spectral energy distributions / /
MusicGroup
Ðnd / /
Organization
California Institute of Technology / University of California / office of Naval Research / Chatterton Astronomy Department / African Union / National Science Foundation / School of Physics / University of Sydney / UC Berkeley / Cambridge Univ. / University of California / Berkeley / National Aeronautics and Space Administration / American Astronomical Society / W. M. Keck Foundation / Smithsonian / /
Person
Van Leeuwen / Min Stellar Temp / Titterington / Anglea (deg) Stellar / Ðtting / Max Stellar Temp / Jean-Pierre Caillautt / Van Belle / Sivia / /
Position
D. J. / model / calibrator / /
Product
Nikon D200 Digital Camera / /
ProvinceOrState
New Mexico / Alabama / California / Massachusetts / Colorado / /
THE ASTROPHYSICAL JOURNAL, 534 : 907È914, 2000 May[removed]The American Astronomical Society. All rights reserved. Printed in U.S.A. NEAR- AND MID-INFRARED SUBARCSECOND STRUCTURE OF THE DUSTY SYMBIOTIC STAR R AQUARII