4.6 Article

The first 8-13 μm spectra of globular cluster red giants:: circumstellar silicate dust grains in 47 Tucanae (NGC 104)

Journal

ASTRONOMY & ASTROPHYSICS
Volume 450, Issue 1, Pages 339-343

Publisher

EDP SCIENCES S A
DOI: 10.1051/0004-6361:20054702

Keywords

stars : AGB and post-AGB; circumstellar matter; stars : evolution; stars : mass-loss; infrared : stars; globular clusters : individual : 47 Tucanae (NGC 104)

Funding

  1. Science and Technology Facilities Council [PP/D000955/1] Funding Source: researchfish
  2. STFC [PP/D000955/1] Funding Source: UKRI

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We present 8-13 mu m spectra of eight red giants in the globular cluster 47 Tucanae (NGC104), 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 V1, shows direct evidence of circumstellar grains made of amorphous silicate.

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