From the atmosphere to the circumstellar environment in cool evolved stars. Issue 69 (10th September 2015)

• Record Type: Journal Article
• Authors: Wittkowski, M.; Paladini, C.
• Editors: Millour, F.; Chiavassa, A.; Bigot, L.; Chesneau, O.; Meilland, A.; Stee, Ph.
• Is Part Of: EAS publications series. Issue 69/70(2014)
• Page Start: 179
• Page End: 195
• Publication Date: 2015-09-10
• Subjects: Astronomy -- Periodicals; 520
• DOI: 10.1051/eas/1569009
• Languages: English
• ISSNs: 1633-4760

Abstract

Abstract : We discuss and illustrate contributions that optical interferometry has made on our current understanding of cool evolved stars. We include red giant branch (RGB) stars, asymptotic giant branch (AGB) stars, and red supergiants (RSGs). Studies using optical interferometry from visual to mid-infrared wavelengths have greatly increased our knowledge of their atmospheres, extended molecular shells, dust formation, and winds. These processes and the morphology of the circumstellar environment are important for the further evolution of these stars toward planetary nebulae (PNe) and core-collapse supernovae (SNe), and for the return of material to the interstellar medium.