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Search for Optical Flashes from the Radio Source CP 1919

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Abstract

The four rapidly pulsating radio sources discovered by Hewish et al. 1 have been tentatively identified with neutron stars or white dwarfs, and their optical identification is therefore of great interest.

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Referenzen

  1. Hewish, A., Bell, S. J., Pilkington, J. D. H., Scott, P. F., and Collins, R. A., Nature, 217, 709 (1968), (Paper 1).

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  2. Ryle, M., and Bailey, J. A., Nature, 217, 907 (1968), (Paper 19).

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  3. Hewish, A., Meeting of the Royal Astronomical Society (London. April 10, 1968).

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  4. Johnson, H. L., Astrophys. J., 116, 640 (1952).

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  5. Davies, J. G., Horton, P. W., Lyne, A. G., Rickett, B. J., and Smith, F. G., Nature, 217, 910 (1968), (Paper 6).

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  6. Radhakrishnan, V., Komesaroff, M. M., and Cooke, D. J., Nature, 218, 229 (1968), (Paper 17).

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© 1968 Springer Science+Business Media New York

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Jelley, J.V., Willstrop, R.V. (1968). Search for Optical Flashes from the Radio Source CP 1919. In: Pulsating Stars. Springer, Boston, MA. https://doi.org/10.1007/978-1-4899-6387-1_25

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  • DOI: https://doi.org/10.1007/978-1-4899-6387-1_25

  • Publisher Name: Springer, Boston, MA

  • Print ISBN: 978-1-4899-6191-4

  • Online ISBN: 978-1-4899-6387-1

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