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https://doi.org/10.1080/10556790412331315815
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Cite Publication Date: Oct 1, 2004 |
Affiliation: Saint Mary's University
Our photoelectric observations of two Mira variables, DW Mus and BI Sco, complemented by ASAS3† survey data, allowed us to construct light curves for these Mira stars as well as to define their current light elements. All Sky Automatic Survey.
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