Dusty LBV nebulae: Tracing the mass loss history of the most massive stars

We present spectra obtained with the Infared Space Observatory (ISO) of the dust shells surrounding several Luminous Blue Variables (LBVs), both in our galaxy and in the LMC. The 20–45 µm spectra of R71, AG Car and Wra 751 show prominent emission features from crystalline silicates. The composition...

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Bibliographische Detailangaben

Hauptverfasser:	Waters, Laurens B. F. M., Voors, Robert H. M., Morris, Patrick W., Trams, Norman R., de Koter, Alex, Lamers, Henny J. G. L.
Format:	Buchkapitel
Sprache:	eng
Schlagworte:	Band Strength Crystalline Silicate Dust Shell Mass Loss Rate Massive Star
Online-Zugang:	Volltext
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