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

J. Th Van Loon, I. McDonald, J. M. Oliveira, A. Evans, M. L. Boyer, Robert D Gehrz, E. Polomski, Chick E Woodward

Research output: Contribution to journalArticlepeer-review

34 Scopus citations

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 languageEnglish (US)
Pages (from-to)339-343
Number of pages5
JournalAstronomy and Astrophysics
Volume450
Issue number1
DOIs
StatePublished - Apr 2006

Keywords

  • Circumstellar matter
  • Globular clusters: individual: 47 Tucanae (NGC 104)
  • Infrared: stars
  • Stars: AGB and post-AGB
  • Stars: evolution
  • Stars: mass-loss

Fingerprint

Dive into the research topics of 'The first 8-13 μm spectra of globular cluster red giants: Circumstellar silicate dust grains in 47 Tucanae (NGC 104)'. Together they form a unique fingerprint.

Cite this