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Fender, R. P., Southwell, K. A., & Tzioumis, A. K. (1998). A radio survey of supersoft transient and persistent X-ray sources in the Magellanic Clouds. Monthly Notices of the Royal Astronomical Society, 298, 692-696. https://doi.org/10.1046/j.1365-8711.1998.01680.x
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Mot, E. S. (1998). Fietsen in de avond. (seo-REEKS; No. 498). SEO. http://HTTP//WWW/TREFPUNT.NL
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Smith, I. A., Hurley, K. C., van Paradijs, J. A., Waters, L. B. F. M., Schulz, A. S. B., Duchouroux, P., Joyce, R., Chernin, L. M., Vrba, F. J., Hartmann, D., Kouveliotou, C., Wallyn, P., & Corbel, S. (1998). Infrared, submillimeter, and millimeter observations of the soft gamma repeaters. Advances in Space Research, 22(7), 1133-1138. https://doi.org/10.1016/S0273-1177(98)00209-9
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Hurley, K. C., Kouveliotou, C., Harmon, B. A., Fishman, G. J., Briggs, M. S., van Paradijs, J. A., Kommers, J. M., Lewin, W. H. G., Cline, T., Boer, M., & Niel, M. (1998). Verifying the accuracy of the third interplanetray network: localization of the bursting pulsar GRO J1744-28 by triangulation. Advances in Space Research, 22(7), 1125-1128. https://doi.org/10.1016/S0273-1177(98)00207-5
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Blommeart, J. A. D. L., Trams, N. R., Okumura, K., Groenewegen, M. A. T., van Loon, J. T., Waters, L. B. F. M., Cioni, M. R., Habing, H. J., Zijlstra, A. A., & Loup, C. (1998). Evolution and mass loss of AGB stars in the Small Magellanic Clouds. In C. Waelkens, L. B. F. M. Waters, K. A. van der Hucht, & P. A. Zaal (Eds.), ISO's view on stellar evolution (pp. 399-400). (Astrophysics and Space Science; No. 255). Kluwer Academic Publishers.
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Méndez, M., van der Klis, M., van Paradijs, J., Lewin, W. H. G., Vaughan, B. A., Kuulkers, E., Zhang, W., Lamb, F. K., & Psaltis, D. (1998). A varying kHz peak seperation in 4U 1608-52. In S. S. Holt, & T. R. Kallman (Eds.), Accretion Processes in Astrophysical Systems: Some Like it Hot!: Eighth Astrophysics Conference, College Park, MD, October 1997 (pp. 385-388). (AIP Conference Proceedings; Vol. 431). American Institute of Physics. https://doi.org/10.1063/1.55922
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