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Results: 384
Number of items: 384
  • Lamers, H. J. G. L. M., Vink, J. S., de Koter, A., & Cassinelli, J. P. (1999). Disks formed by rotation induced bi-stability. In O. Stahl, B. Wolf, & A. Fullerton (Eds.), Variable and non-spherical stellar winds in luminous hot stars (pp. 159-166). Springer.
  • Vink, J. S., de Koter, A., & Lamers, H. J. G. L. M. (1999). Force multipliers and the bistability of stellar winds. In O. Stahl, B. Wolf, & A. Fullerton (Eds.), Variable and non-spherical stellar winds in luminous hot stars (pp. 132). Springer.
  • Morris, P. W., Waters, L. B. F. M., Barlow, M. J., Lim, T., de Koter, A., Voors, R. H. M., Cox, P., de Graauw, T., Henning, T., Hony, S., Lamers, H. J. G. L. M., Mutschke, H., & Trams, N. R. (1999). Discovery of a massive equatorial torus in the eta Carinae stellar system. Nature, 402, 502-504. https://doi.org/10.1038/990048
  • Molster, F. J., Yamamura, I., Waters, L. B. F. M., Tielens, A. G. G. M., de Graauw, T., de Jong, T., de Koter, A., Malfait, K., van den Ancker, M. E., van Winckel, H., Voors, R. H. M., & Waelkens, C. (1999). Low-temperature crystallization of silicate dust in circumstellar disks. Nature, 401, 563-565. https://doi.org/10.1038/44085
  • de Koter, A., Vink, J. S., & Lamers, H. J. G. L. M. (1999). Spectroscopic dating of very massive stars. In S. R. Heap, I. Hubeny, & R. Cornett (Eds.), Spectrophotometric dating of stars and galaxies (Vol. 192, pp. 32-40). ASP.
  • Waters, L. B. F. M., Voors, R. H. M., Morris, P. W., Trams, N. R., de Koter, A., & Lamers, H. J. G. L. M. (1999). Dust in LBV nebulae: tracing the mass loss history of the most massive stars. In O. Stahl, B. Wolf, & A. W. Fullerton (Eds.), Variable and non-spherical stellar winds in luminous hot stars (pp. 381-390). Springer.
  • Trams, N. R., van Tuyll, C., Voors, R. H. M., de Koter, A., Waters, L. B. F. M., & Morris, P. W. (1999). Non-isotropic outflows in the infrared: ISO imaging of LVBs. In O. Stahl, B. Wolf, & A. Fullerton (Eds.), Variable and non-spherical stellar winds in luminous hot stars (pp. 71-79). Springer.
  • De Marco, O., Schmutz, W., Koesterke, L., Hamann, W. R., & de Koter, A. (1999). Why should we compare Wolf-Rayet codes? In G. Koenigsberger, K. A. van der Hucht, & P. R. J. Eenens (Eds.), Wolf-Rayet phenomena in massive stars and starburst galaxies (pp. 231-232). ASP.
  • De Marco, O., Schmutz, W., & de Koter, A. (1999). Gamma Velorum, photon loss and the velocity field. In G. Koenigsberger, K. A. van der Hucht, & P. R. J. Eenens (Eds.), Wolf-Rayet phenomena in massive stars and starburst galaxies (pp. 229-230). ASP.
  • Morris, P. W., Bouwman, J., Crowther, P. A., Dessart, L., van der Hucht, K. A., de Koter, A., Kudritzki, R. P., Lamers, H. J. G. L. M., Najarro, F., Trams, N. R., van Tuyll, C., Voors, R. H. M., Waters, L. B. F. M., Williams, P. M., & Willis, A. J. (1999). ISO studies of luminous, early-type stars. In M. F. Kessler, & P. Cox (Eds.), The universe as seen by ISO (Vol. 427, pp. 247-255). ESA.
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