Carbonaceous molecules in the oxygen-rich circumstellar environment of binary post-AGB stars-C60 fullerenes and polycyclic aromatic hydrocarbons
- Authors
- Type
- Published Article
- Journal
- ScienceOpen Astronomy & Astrophysics
- Publisher
- ScienceOpen
- Publication Date
- Dec 01, 2011
- Volume
- 536
- Pages
- 54–54
- Source
- SETI Institute
- License
- Unknown
Abstract
Context. The circumstellar environment of evolved stars is generally rich in molecular gas and dust. Typically, the entire environment is either oxygen-rich or carbon- rich, depending on the evolution of the central star. Aims. In this paper we discuss three evolved disc sources with evidence of atypical emission lines in their infrared spectra. The stars were taken from a larger sample of post-AGB binaries for which we have Spitzer infrared spectra, characterised by the presence of a stable oxygen-rich circumbinary disc. ...