Dust features in the 10-mu m infrared spectra of oxygen-rich evolved stars

By A. Speck, M. Barlow, R. Sylvester, Anne M. Hofmeister. 2000

159 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/3e15c1edd5ed0b175073f7f82edc8211a03a29bb

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. D. Clayton
2. Th. Henning
3. L. Nittler
4. K. Meisenheimer
5. V. Hamilton
6. C. Mordasini
7. Anders Johansen
8. A. Youdin

In Instrumentation

1. Th. Henning
2. L. Nittler
3. K. Meisenheimer

Citations in the corpus

• Steps toward interstellar silicate mineralogy - VII. Spectral properties and crystallization behaviour of magnesium silicates produced by the sol-gel method (2003, methodology): “Speck et al. (2000) have used UKIRT CGS3 spectra in order to classify the 10µm profiles of AGB stars and supergiants into characteristic groups.”
• Resolving the obscuring torus in NGC 1068 with the power of infrared interferometry: revealing the inner funnel of dust (2009, methodology): “We have selected several dust absorption templates, including standard galactic dust as observed towards the centre of the Milky Way (Kemper et al. 2004), as well as Ca2Al 2SiO7 , which was found to best fit the previous MIDI data (J04, Speck et al. (2000)).”
• Astrophysics with Presolar Stardust (2004, background): “…features associated with specific dust species are observed around many evolved stars, including silicate and oxide features in O-rich stars (Speck et al. 2000, Waters et al. 1996) and an 11.3 µm SiC feature in many C stars (Blanco et al. 1998, 22 Speck & Hofmeister 2003, Treffers & Cohen…”
• Probing the mass-loss history of AGB and red supergiant stars from CO rotational line profiles. II. CO line survey of evolved stars: derivation of mass-loss rate formulae (2010, unknown): “The low luminosity and the dust features in the ISO spectrum make classification of T Cet as AGB star more plausible (Speck et al. 2000; Verhoelst et al. 2009).”
• Presolar stardust in meteorites : recent advances and scientific frontiers (2003, background): “Infrared spectroscopic features of SiC and corundum have also been observed around such stars [28,29].”