Abstract
We present 8-13 μm spectra of eight red giants in the globular cluster 47 Tucanae (NGC 104), obtained at the European Southern Observatory 3.6 m telescope. These are the first mid-infrared spectra of metal-poor, low-mass stars. The spectrum of at least one of these, namely the extremely red, large-amplitude variable VI, shows direct evidence of circumstellar grains made of amorphous silicate.
Original language | English (US) |
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Pages (from-to) | 339-343 |
Number of pages | 5 |
Journal | Astronomy and Astrophysics |
Volume | 450 |
Issue number | 1 |
DOIs | |
State | Published - Apr 2006 |
Keywords
- Circumstellar matter
- Globular clusters: individual: 47 Tucanae (NGC 104)
- Infrared: stars
- Stars: AGB and post-AGB
- Stars: evolution
- Stars: mass-loss