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The spectroscopic identification of interstellar grains

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Abstract

It is shown that the condition of matching the 3.3–3.9 μm spectrum of the galactic infrared source GC-IRS 7 leads to a remarkably tight convergence on the transmittance curve measured in the laboratory for the dessicated bacteriumE. coli. Other materials, including certain biochemicals and postulated prebiologic compounds, are shown to be deficient with regard to meeting this condition.

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References

  • Allen, D. A. and Wickramasinghe, D. T.: 1981,Nature 294, 239.

    Google Scholar 

  • Engels, M. E. and Nagy, B.: 1982,Nature 296, 837.

    Google Scholar 

  • Greenberg, J. M.: 1982, in L. L. Wilkening (ed.),Comets, University of Arizona Press.

  • Hoyle, F., Wickramasinghe, N. C., Olavesen, A. H., Al-Mufti, S., and Wickramasinghe, D. T.: 1982,Astrophys. Space Sci. 83, 405.

    Google Scholar 

  • Khare, B. N. and Sagan, C.: 1973,Icarus 20, 311.

    Google Scholar 

  • Moore, M. H. and Donn, B.: 1982,Astrophys. J. 257, L47.

    Google Scholar 

  • Pflug, H. D.: 1982, private communication.

  • Pflug, H. D.: 1984, in C. Wickramasinghe (ed.),Fundamental Studies and the Future of Science, U.C.C. Press.

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Hoyle, F., Wickramasinghe, N.C. & Al-Mufti, S. The spectroscopic identification of interstellar grains. Astrophys Space Sci 98, 343–352 (1984). https://doi.org/10.1007/BF00651413

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  • DOI: https://doi.org/10.1007/BF00651413

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