Dust-enshrouded giants in clusters in the Magellanic Clouds

We present the results of an investigation of post-Main Sequence mass loss from stars in clusters in the Magellanic Clouds, based around an imaging survey in the $L^\prime$-band (3.8 μm) performed with the VLT at ESO. The data are complemented with ${\it JHK}_{\rm s}$ (ESO and 2MASS) and mid-IR phot...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2005-11, Vol.442 (2), p.597-613
Hauptverfasser:	van Loon, J. Th, Marshall, J. R., Zijlstra, A. A.
Format:	Artikel
Sprache:	eng
Schlagworte:	infrared: stars Magellanic Clouds stars: AGB and post-AGB stars: mass-loss Sun: evolution supergiants
Online-Zugang:	Volltext
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