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Schuller, P., Salomé, P., Perrin, G., Mennesson, B., Niccolini, G., de Laverny, P., Ridgway, S. T., V. Coudé du Foresto, , Traub, W. A. (2004) Are dust shell models well-suited to explain interferometric data of late-type stars in the near-infrared?. Astronomy & Astrophysics, 418 (1). 151-162 doi:10.1051/0004-6361:20040057

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Reference TypeJournal (article/letter/editorial)
TitleAre dust shell models well-suited to explain interferometric data of late-type stars in the near-infrared?
JournalAstronomy & Astrophysics
AuthorsSchuller, P.Author
Salomé, P.Author
Perrin, G.Author
Mennesson, B.Author
Niccolini, G.Author
de Laverny, P.Author
Ridgway, S. T.Author
V. Coudé du Foresto, Author
Traub, W. A.Author
Year2004 (April)Volume418
Issue1
PublisherEDP Sciences
DOIdoi:10.1051/0004-6361:20040057Search in ResearchGate
Generate Citation Formats
Mindat Ref. ID3462647Long-form Identifiermindat:1:5:3462647:2
GUID0
Full ReferenceSchuller, P., Salomé, P., Perrin, G., Mennesson, B., Niccolini, G., de Laverny, P., Ridgway, S. T., V. Coudé du Foresto, , Traub, W. A. (2004) Are dust shell models well-suited to explain interferometric data of late-type stars in the near-infrared?. Astronomy & Astrophysics, 418 (1). 151-162 doi:10.1051/0004-6361:20040057
Plain TextSchuller, P., Salomé, P., Perrin, G., Mennesson, B., Niccolini, G., de Laverny, P., Ridgway, S. T., V. Coudé du Foresto, , Traub, W. A. (2004) Are dust shell models well-suited to explain interferometric data of late-type stars in the near-infrared?. Astronomy & Astrophysics, 418 (1). 151-162 doi:10.1051/0004-6361:20040057
In(2004, April) Astronomy & Astrophysics Vol. 418 (1) EDP Sciences

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