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Spectral speckle interferometry

  • Seventh Session Interferometry
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Abstract

A method of obtaining an objective prism spectrum of a stellar object with diffraction-limited spatial resolution is described.

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References

  • Baba, N. and Tabata, M.: 1988, in F. Merkle (ed.),High Resolution Imaging by Interferometry, Garching.

  • Baba, N., Tabata, M., and Murata, K.:1988,Opt. Letters 13, 616.

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  • Bates, R. H. T. and Cady, F. M.: 1980,Opt. Commun. 32, 365.

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  • Grieger, F., Fleischmann, F., and Weigelt, G.: 1988, in F. Merkle (ed.),High Resolution Imaging by Interferometry, Garching.

  • Ribak, E., Hege, E. K., and Christou, J. C.: 1985,Proc. Soc. Photo-Opt. Instrum. Eng. 556, 196.

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  • Weigelt, G.: 1981,Proc. Scientific Importance of High Angular Resolution at IR and Optical Wavelength, ESO Conf.

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Authors and Affiliations

  1. Hokkaido University, Sapporo, Japan

    Naoshi Baba

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  1. Naoshi Baba
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Baba, N. Spectral speckle interferometry. Astrophys Space Sci 160, 373–376 (1989). https://doi.org/10.1007/BF00642794

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  • DOI: https://doi.org/10.1007/BF00642794

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