Search results
Results: 167
Number of items: 167
-
Migliari, S., di Salvo, T., Belloni, T., van der Klis, M., Fender, R. P., Campana, S., Kouveliotou, C., Méndez, R. M., & Lewin, W. H. G. (2003). Discovery of type I X-ray bursts from the low-mass X-ray binary 4U 1708-40. Monthly Notices of the Royal Astronomical Society, 342(3), 909-914. https://doi.org/10.1046/j.1365-8711.2003.06597.x
-
Patel, S. K., Kouveliotou, C., Woods, P. M., Tennant, A., Weisskopf, M. C., Finger, M. H., Wilson, C. A., Gogus, E., van der Klis, M., & Belloni, T. (2003). Chandra Observations of the Anomalous X-ray Pulsars 1E 2259+586 and 4U 0142+61. In G. Cusumano, E. Massaro, & T. Mineo (Eds.), Pulsars, AXPs and SGRs observed with BeppoSAX and Other Observatories (pp. 207-214). Aracne Editrice.
-
Migliari, S., & Belloni, T. (2003). Evidence for local mass accretion rate variations in the disc of GRS 1915+105. Astronomy & Astrophysics, 404, 283-289. https://doi.org/10.1051/0004-6361:20030484 -
Nespoli, E., Belloni, T., Homan, J., Miller, J. M., Lewin, W. H. G., Méndez, R. M., & van der Klis, M. (2003). A transient variable 6 Hz QPO from GX 339-4. Astronomy & Astrophysics, 412, 235-240. https://doi.org/10.1051/0004-6361:20031423 -
Reig, P., Belloni, T., & van der Klis, M. (2003). Does GRS 1915+105 exhibit ``canonical'' black-hole states? Astronomy & Astrophysics, 412, 229-233. https://doi.org/10.1051/0004-6361:20031388 -
Wilson, C. A., Patel, S. K., Kouveliotou, C., Jonker, P. G., van der Klis, M., Lewin, W. H. G., Belloni, T., & Méndez, R. M. (2003). Chandra Observations of the Faintest Low-Mass X-Ray Binaries. Astrophysical Journal, 596(2), 1220-1228. https://doi.org/10.1086/377473 -
Jonker, P. G., van der Klis, M., Kouveliotou, C., Méndez, R. M., Lewin, W. H. G., & Belloni, T. (2003). MS 1603.6+2600: an accretion disc corona source? Monthly Notices of the Royal Astronomical Society, 346(2), 684-688. https://doi.org/10.1046/j.1365-2966.2003.07123.x -
Vignarca, F., Migliari, S., Belloni, T., Psaltis, D., & van der Klis, M. (2003). Tracing the power-law component in the energy spectrum of black hole candidates as a function of the QPO frequency. Astronomy & Astrophysics, 397, 729-738. https://doi.org/10.1051/0004-6361:20021542
Page 9 of 17