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Results: 371
Number of items: 371
  • Jensen, B. L., Hjorth, J., Pritchard, J., Pedersen, H., Masetti, N., Palazzi, E., Gorosabel, J., Castro-Tirado, A. J., Salvato, M., Kouveliotou, C., Rol, E., Kaper, L., Zapatero-Osario, M. R., & Rosenberg, A. (2000). GRB 000115 Optical observations. GRB Coordinates Network, Circular Service, 524.
  • Kaper, L. (2000). Observations of the wind structure of OB-type stars. In H. J. G. L. M. Lamers, & A. Sapar (Eds.), Thermal and ionization aspects of flows from hot stars: observations and theory (Vol. 204, pp. 3-14). ASP Conference Series.
  • Kaper, L., Comeron, F., & Hanson, M. M. (2000). Probing the young OB stars in ultra-compact H II regions. In F. Favata, A. Kaas, & A. Wilson (Eds.), Proc. 33rd ESLAB Symp. "Star formation from the small to the large scale" (pp. 433-436). Estec.
  • Lenorzer, A., Vandenbussche, B., de Koter, A., Kaper, L., Waters, L. B. F. M., & Morris, P. W. (2000). Infrared 2.4-4.1 micron spectra of OB-type stars. In A. Salama, & M. F. Kessler (Eds.), ISO beyond the peaks (Vol. 456, pp. 211-214). ESA-SP.
  • Henrichs, H. F., de Jong, J. A., Donati, J. F., Catala, C., Wade, G. A., Shorlin, S. L. S., Veen, P. M., Nichols, J. S., & Kaper, L. (2000). The Magnetic Field of beta Cep and the Be Phenomenon. In M. A. Smith, H. F. Henrichs, & J. Fabregat (Eds.), The Be Phenomenon in Early-Type Stars, IAU Colloquium 175 (Vol. 214, pp. 324-329). ASP Conference Series.
  • Henrichs, H. F., de Jong, J. A., Donati, J. F., Wade, G. A., Babel, J., Shorlin, S. L. S., Verdugo, E., Talavera, A., Catala, C., Veen, P. M., Nichols, J. S., & Kaper, L. (2000). Detection of a weak magnetic field in the pulsating Be star beta Cephei. In Y. V. Glagolevskij, & I. I. Romanyuk (Eds.), Magnetic Fields of Chemically Peculiar and Related Stars, Special Astrophysical Observatory of Russian AS (pp. 57-60)
  • Open Access
    Rol, E., Wijers, R. A. M. J., Vreeswijk, P. M., Kaper, L., Galama, T. J., van Paradijs, J. A., Kouveliotou, C., Masetti, N., Pian, E., Palazzi, E., Frontera, F., & van den Heuvel, E. P. J. (2000). GRB 990712: First Indication of Polarization Variability in a Gamma-Ray Burst Afterglow. Astrophysical Journal, 544(2), 707-711. https://doi.org/10.1086/317256
  • Open Access
    van den Heuvel, E. P. J., Portegies Zwart, S. F., Bhattacharya, D., & Kaper, L. (2000). On the origin of the difference between the runaway velocities of the OB-supergiant X-ray binaries and the BE/X-ray binaries. Astronomy & Astrophysics, 364, 563-572. http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2000A%26A...364..563V&db_key=AST
  • Open Access
    Andersen, M. I., Hjorth, J., Pedersen, H., Jensen, B. L., Hunt, L. K., Gorosabel, J., Moeller, P., Fynbo, J., Kippen, R. M., Thomsen, B., Olsen, L. F., Christensen, L., Vestergaard, M., Masetti, N., Palazzi, E., Hurley, K., Cline, T., Kaper, L., & Jaunsen, A. O. (2000). VLT identification of the optical afterglow of the gamma-ray burst GRB 000131 at z=4.50. Astronomy & Astrophysics, 364, L54-L61.
  • Kaper, L. (1999). O-star wind variability in the UV and optical range. In A. W. Fullerton, B. Wolf, & O. Stahl (Eds.), Variable and non-spherical stellar winds in luminous hot stars (Vol. 523, pp. 193-200). Springer.
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