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This article has been cited by the following article(s):
THE MASS-LOSS RETURN FROM EVOLVED STARS TO THE LARGE MAGELLANIC CLOUD. IV. CONSTRUCTION AND VALIDATION OF A GRID OF MODELS FOR OXYGEN-RICH AGB STARS, RED SUPERGIANTS, AND EXTREME AGB STARS
THE ARIZONA RADIO OBSERVATORY 1 mm SPECTRAL SURVEY OF IRC +10216 AND VY CANIS MAJORIS (215–285 GHz)
E. D. Tenenbaum, J. L. Dodd, S. N. Milam, N. J. Woolf and L. M. Ziurys The Astrophysical Journal Supplement Series 190(2) 348 (2010) https://doi.org/10.1088/0067-0049/190/2/348
Probing the mass-loss history of AGB and red supergiant stars from CO rotational line profiles