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Results: 684
Number of items: 684
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Wijnands, R. A. D., Guainazzi, M., van der Klis, M., & Méndez, R. M. (2002). XMM-Newton Observations of the Neutron Star X-Ray Transient KS 1731-260 in Quiescence. Astrophysical Journal, 573(1), L45-L49. https://doi.org/10.1086/341960
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Jonker, P. G., van der Klis, M., Homan, J., Méndez, R. M., Lewin, W. H. G., Wijnands, R. A. D., & Zhang, W. (2002). Low- and high-frequency variability as a function of spectral properties in the bright X-ray binary GX 5-1. Monthly Notices of the Royal Astronomical Society, 333(3), 665-678. https://doi.org/10.1046/j.1365-8711.2002.05442.x -
Corbel, S., Fender, R. P., Tzioumis, A. K., Tomsick, J. A., Orosz, J. A., Miller, J. M., Wijnands, R. A. D., & Kaaret, P. (2002). Moving relativistic large-scale X-ray jets in the microquasar XTE J1550-564. In P. Durouchoux, Y. Fuchs, & J. Rodriguez (Eds.), New Views on MICROQUASARS (pp. 197). Center for Space Physics.
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Tomsick, J. A., Corbel, S., Fender, R. P., Miller, J. M., Orosz, J. A., Tzioumis, A. K., Wijnands, R. A. D., & Kaaret, P. (2002). X-ray jet emission from the black hole X-ray binary XTE J1550-564 with CHANDRA in 2000. In P. Durouchoux, Y. Fuchs, & J. Rodriguez (Eds.), New Views on MICROQUASARS (pp. 221). Center for Space Physics.
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Homan, J., van der Klis, M., Jonker, P. G., Wijnands, R., Kuulkers, E., Méndez, M., & Lewin, W. H. G. (2002). RXTE Observations of the Neutron Star Low-Mass X-Ray Binary GX 17+2: Correlated X-Ray Spectral and Timing Behavior. Astrophysical Journal, 568(2), 878-900. https://doi.org/10.1086/339057
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Wijnands, R. A. D., Miller, J. M., & van der Klis, M. (2002). 4U 1957+11: a persistent low-mass X-ray binary and black hole candidate in the high state? Monthly Notices of the Royal Astronomical Society, 331(1), 60-70. https://doi.org/10.1046/j.1365-8711.2002.05137.x -
Corbel, S., Fender, R. P., Tzioumis, A. K., Tomsick, J. A., Orosz, J. A., Miller, J. M., Wijnands, R. A. D., & Kaaret, P. (2002). Large-Scale, Decelerating, Relativistic X-ray Jets from the Microquasar XTE J1550-564. Science, 298(5591), 196-199. https://doi.org/10.1126/science.1075857
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