A VISIR Mid-infrared Imaging Survey of Post-AGB Stars

Details A VISIR Mid-infrared Imaging Survey of Post-AGB Stars A VISIR Mid-infrared Imaging Survey of Post-AGB Stars

Jun 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011msngr.144...21l&link_type=abstract

The Messenger, vol. 144, p. 21-24

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Post asymptotic giant branch (AGB) stars are key objects for the study of the dramatic morphological changes that low- to intermediate-mass stars undergo during their evolution from the AGB towards the planetary nebula stage. There is growing evidence that binary interaction processes may play a determining role in shaping many objects, but so far direct evidence for binarity is still weak. We report on a systematic study of the dust distribution around a large sample of post-AGB stars that probes the symmetry-breaking in the nebulae around these systems.

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