The Size, Structure, and Variability of Late-Type Stars Measured ...
The Size, Structure, and Variability of Late-Type Stars Measured ...
The Size, Structure, and Variability of Late-Type Stars Measured ...
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[92] Martin Schwarzschild. Overtone pulsations for the st<strong>and</strong>ard model. <strong>The</strong> Astrophysical<br />
Journal, 94:245–252, 1941.<br />
[93] M. Shao <strong>and</strong> M. M. Colavita. Long-baseline optical <strong>and</strong> infrared stellar interferometry.<br />
Annual Review <strong>of</strong> Astronomy <strong>and</strong> Astrophysics, 30:457–498, 1992.<br />
[94] W. B. Somerville. <strong>The</strong> continuous absorption coefficient <strong>of</strong> the negative hydrogen<br />
molecular ion. <strong>The</strong> Astrophysical Journal, 139:192–197, 1964.<br />
[95] C. Sterken, E. Broens, <strong>and</strong> C. Koen. On the period history <strong>of</strong> χ cygni. Astronomy<br />
<strong>and</strong> Astrophysics, 342:167–172, 1999.<br />
[96] Kyung-Won Suh. Optical properties <strong>of</strong> the silicate dust grains in the envelopes around<br />
asymptotic giant branch stars. Mon. Not. R. Astron. Soc., 304:389–405, April 1999.<br />
[97] R. R. Thompson, M. J. Creech-Eakman, <strong>and</strong> R. L. Akeson. Time-dependent asymmetries<br />
in the atmosphere <strong>of</strong> the mira variable r trianguli through infrared interferometry.<br />
<strong>The</strong> Astrophysical Journal, 570:373–378, May 2002.<br />
[98] R. R. Thompson, M. J. Creech-Eakman, <strong>and</strong> G. T. van Belle. Multiepoch interferometric<br />
study <strong>of</strong> mira variables. i. narrowb<strong>and</strong> diameters <strong>of</strong> rz pegasi <strong>and</strong> s lacertae.<br />
<strong>The</strong> Astrophysical Journal, 577:447–456, September 2002.<br />
[99] T. Tsuji. Water on the early m supergiant stars α orionis <strong>and</strong> µ cephei. <strong>The</strong> Astophysical<br />
Journal, 538:801–807, August 2000.<br />
[100] T. Tsuji. Water in k <strong>and</strong> m giant stars unveiled by iso. Astronomy <strong>and</strong> Astrophysics,<br />
376:L1–L4, 2001.<br />
[101] Y. Tuchman. <strong>The</strong>oretical pulsation models for long period variables. In T. Le Bertre,<br />
A. Lebre, <strong>and</strong> C. Waelkens, editors, Proc. I. A. U. Symposium. 191, Asymptotic Giant<br />
Branch <strong>Stars</strong>, pages 123–131, 1999.<br />
[102] P. G. Tuthill, C. A. Haniff, <strong>and</strong> J. E. Baldwin. Long-term diameter variations in the<br />
long-period variable o ceti. Mon. Not. R. Astron. Soc., 277:1541–1546, 1995.<br />
[103] P. G. Tuthill, C. A. Haniff, <strong>and</strong> J. E. Baldwin. Hotspots on late-type supergiants.<br />
Mon. Not. R. Astron. Soc., 285:529–539, March 1997.