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Q53951855-0B1A37DC-5307-4287-B601-06C80EE98ADF
Q53951855-0B1A37DC-5307-4287-B601-06C80EE98ADF
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http://www.wikidata.org/entity/statement/Q53951855-0B1A37DC-5307-4287-B601-06C80EE98ADF
What causes the large extensions of red supergiant atmospheres? Comparisons of interferometric observations with 1D hydrostatic, 3D convection, and 1D pulsating model atmospheres
P2860
Q53951855-0B1A37DC-5307-4287-B601-06C80EE98ADF
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http://www.wikidata.org/entity/statement/Q53951855-0B1A37DC-5307-4287-B601-06C80EE98ADF
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da7b87e5efd7f4774450a7f2617ca35c0886cbdd
P2860
The Mira variable S Orionis: relationships between the photosphere, molecular layer, dust shell, and SiO maser shell at 4 epochs