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Optical constants of cosmic carbon analogue grains — I. Simulation of clustering by a modified continuous distribution of ellipsoids
Abstract
The first results on the optical constants of three different amorphous carbon samples, possible analogues of interstellar and circumstellar dust grains, are presented. They have been deduced from recent laboratory data, making use of the Kramers-Kronig approach. It is shown that the physically correct simulation of clustering by the traditional ‘CDE’ model is not applicable here. A modified CDE (MCDE) model is proposed and used in the present calculations. The MCDE model allows one to take into account the effect of percolation of the analysed amorphous carbon clusters through the parameter go, interpreted as a percolation strength. The intervals of the probable MCDE models (go) have been chosen on the basis of the relevant estimates of Stognienko, Henning & Ossenkopf for the cluster—cluster aggregation (CCA) and particle—cluster aggregation (PCA) models. The ‘optimal’ percolation strengths and optical constants have been derived by using a least-squares procedure.
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Cites
Absorption and Scattering of Light by Small Particles
Bohren, C. F., & Huffman, D. R. (1998) · doi:10.1002/9783527618156 · Cited by 18,474
Electrodynamics of Continuous Media
Landau, L. D., Lifshitz, E. M., & King, A. L. (1961) · American Journal of Physics · doi:10.1119/1.1937882 · Cited by 10,997
Cited by
Dust formation and survival in supernova ejecta
Bianchi, S., & Schneider, R. (2007) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2007.11829.x · Cited by 401
Woitke, P., Min, M., Pinte, C., Thi, W.-F., Kamp, I., Rab, C., Anthonioz, F., Antonellini, S., Baldovin-Saavedra, C., Carmona, A., et al. (2016) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201526538 · Cited by 380
Ammoniated phyllosilicates with a likely outer Solar System origin on (1) Ceres
De Sanctis, M. C., Ammannito, E., Raponi, A., Marchi, S., McCord, T. B., McSween, H. Y., Capaccioni, F., Capria, M. T., Carrozzo, F. G., Ciarniello, M., et al. (2015) · Nature · doi:10.1038/nature16172 · Cited by 346
The global dust SED: Tracing the nature and evolution of dust with DustEM
Compiègne, M., Verstraete, L., Jones, A. P., Bernard, J.-P., Boulanger, F., Flagey, N. J., Bourlot, J. L., Paradis, D., & Ysard, N. (2010) · Springer Link (Chiba Institute of Technology) · doi:10.1051/0004-6361/201015292/pdf · Cited by 312
Fabian, D., Henning, T., Jäger, C., Mutschke, H., Dorschner, J., & Wehrhan, O. (2001) · Astronomy & Astrophysics · doi:10.1051/0004-6361:20011196 · Cited by 268
Metadata
- Authors
- Zubko, V. G., Mennella, V., Colangeli, L., & Bussoletti, E.
- Venue
- Monthly Notices of the Royal Astronomical Society
- Publisher
- Oxford University Press (OUP)
- Published
- 1996-10
- Volume
- 282
- Issue
- 4
- Pages
- 1321-1329
- ISSN
- 0035-8711 (ISSN-L)
- 1365-2966
- OpenAlex
- W2050965589
- Cited by
- 580
- References
- 2
- FWCI
- 2.18
- Type
- journal article
- Language
- en
- Open access
- closed
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- Zubko, V. G., Mennella, V., Colangeli, L., & Bussoletti, E. (1996). Optical constants of cosmic carbon analogue grains — I. Simulation of clustering by a modified continuous distribution of ellipsoids. Monthly Notices of the Royal Astronomical Society. https://doi.org/10.1093/mnras/282.4.1321
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