Studying the Pulsation of Mira Variables in the Ultraviolet

Author:

Wood B. E.,Karovska M.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference35 articles.

1. Bevington, P. R. & Robinson, D. K. 1992, Data Reduction and Error Analysis for the Physical Sciences (New York: McGraw-Hill)

2. MG II line profiles of the Mira S Carinae

3. Dynamical modeling of long-period variable star atmospheres

4. Brugel, E. W., Willson, L. A. & Bowen, G. 1990, in Evolution in Astrophysics: IUE Astronomy in the Era of New Space Missions (ESA SP-310; Noordwijk: ESA), 241

5. Brugel, E. W., Willson, L. A. & Cadmus, R. 1986, in New Insights in Astrophysics: Eight Years of UV Astronomy with IUE (ESA SP-263; Noordwijk: ESA), 213

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3. Light curves, variations in the MgII h and k and MgI (2852 Å) emission lines, and polarization of light from the mirids;Astrophysics;2012-09

4. DENSITY EFFECTS ON Mg II EMISSION LINES OF MIRA AB;The Astronomical Journal;2009-02-12

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