Optical properties of circumstellar dust grains

Optical constants derived by Kyung-Won Suh

  1. Suh, Kyung-Won 2016, Optical properties of amorphous alumina dust in the envelopes around O-rich AGB stars, Journal of the Korean Astronomical Society, vol.49, no.4, p.127-136. ADS Link.
    2. Optical constants for amorphous alumina (Al2O3) dust. It lists wavelength(micron), n, k (104 rows). (Density = 3.2 g/cc for amorphous alumina dust)
  2. Suh, Kyung-Won 2000, Optical properties of the carbon dust grains in the envelopes around AGB stars, Monthly Notices of the Royal Astronomical Society, 315, 740-750. ADS Link.
    3. Optical constants for amorphous carbon. It lists wavelength(micron), n, k (98 rows). (Density = 2.0 g/cc for amorphous carbon)
  3. Suh, Kyung-Won 1999, Optical properties of the silicate dust grains in the envelopes around AGB stars, Monthly Notices of the Royal Astronomical Society, 304, 389-405. ADS Link.
    4. Optical constants for warm silicate. It lists wavelength(micron), n, k (98 rows). Optical constants for cold silicate. It lists wavelength(micron), n, k (98 rows). (Density = 3.3 g/cc for silicate)

Links for other sites related with optical properties of dust grains

  1. Databases of Dust Optical Constants at UNIVERSITY OBSERVATORY JENA
  • Kyung-Won Suh's Home Page