Steps toward interstellar silicate mineralogy - VII. Spectral properties and crystallization behaviour of magnesium silicates produced by the sol-gel method

By C. Jäger, J. Dorschner, H. Mutschke, T. Posch, Th. Henning. 2003

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View Paper: https://www.semanticscholar.org/paper/35727e35ed97afef2c2690d637c1c4d0bc129eb3

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In Astronomy and Astrophysics

Citations in the corpus

Low-Temperature Opacities (2005, methodology): “An excellent reference to an online database is found in Jäger et al. (2003b).”
The Absence of Crystalline Silicates in the Diffuse Interstellar Medium (2004, methodology): “For more details, the reader is referred to the work by Jäger et al. (2003a).”
Dust formation and survival in supernova ejecta (2007, unknown): “…Shepherd et al. (1985) 3.74 102 2.32 (30, 80] Koenitzer et al. (1989) 1.04 105 1.04 (80, 300] 3.95 107 0 (300,∞) MgSiO3 9.22 3 (0, 20] Kelley (1943) Jäger et al. (2003) 2.01 3.51 (20, 50] Chase et al. (1985) 7.94 102 1.98 (50, 130] Krupka et al. (1985) 1.32 105 0.93 (130, 400] 3.47 107 0…”
Production of dust by massive stars at high redshift (2011, background): “…constants are taken from Draine and Lee (1984), Draine (1985), Ossenkopf et al (1992) or Laor and Draine (1993), (ii) for Mg protosilicates from Dorschner et al (1980a) or J¨ager et al (2003) and (iii) for amorphous carbon grains values from Hanner (1988) or Rouleau and Martin (1991) are assumed.”
THE TW Hya DISK AT 870 μm: COMPARISON OF CO AND DUST RADIAL STRUCTURES (2011, methodology): “Based on the efforts of Uchida et al. (2004) to faithfully reproduce the details of the Spitzer IRS spectrum, we let 25% of the total silicate abundance inside the disk cavity (r ≤ rcav) be composed of crystalline forsterite (using optical constants from Jäger et al. 2003).”
Freshly Formed Dust in the Cassiopeia A Supernova Remnant as Revealed by the Spitzer Space Telescope (2007, methodology): “We also fit the observations using Mg2SiO4, which exhibits a feature around 20 m and the overall variation of absorption coefficients of Mg2SiO4 whose wavelength might be similar, to that of Mg protosilicate (Dorschner et al. 1980; Jäger et al. 2003).”