Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
1780018 | New Astronomy Reviews | 2009 | 6 Pages |
Abstract
This is a short review of optical interferometry studies involving the VLTI in the field of evolved stars. The various aspects of mass loss from these stars can be followed from the photosphere to the wind, and then to the circumstellar medium. Of particular importance is the possibility offered by this technique to characterize disks of dust or plasma.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Astronomy and Astrophysics
Authors
Olivier Chesneau,