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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Date: 2005-06-13 11:11:58 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. Add to Reading List Source URL: isi.ssl.berkeley.edu Download Document from Source Website File Size: 100,89 KB Share Document on Facebook

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