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Astronomy / Hydroxides / Stellar astronomy / Spectroscopy / Star / Astronomical spectroscopy / Infrared / Protoplanetary nebula / Sun / Electromagnetic radiation / Light sources / Chemistry


The Astrophysical Journal, 611:L37–L40, 2004 August 10 䉷 2004. The American Astronomical Society. All rights reserved. Printed in U.S.A. MIRA’S APPARENT SIZE VARIATIONS DUE TO A SURROUNDING SEMIOPAQUE H2O LAYER J.
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Document Date: 2005-06-13 11:11:58


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City

San Francisco / /

Company

Hale D. D. / /

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Facility

Weiner Space Sciences Laboratory / University of California at Berkeley / Infrared Telescope Facility / /

IndustryTerm

energy levels / /

Organization

Betty Moore Foundation / University of California / office of Naval Research / American Astronomical Society / Department of Physics / National Science Foundation / SURROUNDING SEMIOPAQUE H2O LAYER J. Weiner Space Sciences Laboratory / /

Person

Guy Perrin / Jason Aufdenberg / John Monnier / MIRA COMPARED / John Lacy / Peter Tuthill / Matt Richter / /

/

Position

cohesive model of Mira / THE H2O SHELL MODEL The model / /

PublishedMedium

The Astrophysical Journal / /

Technology

spectroscopy / /

SocialTag