Titlebook: Microquasars; Proceedings of the T A. J. Castro-Tirado,J. Greiner,J. M. Paredes Conference proceedings 2001 Springer Science+Business Media

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The Moderate and High-Speed Photometry of the Black Hole Candidate XTE J1118+480Our March–May photometry of the optical counterpart of the black hole candidate XTE Jl 118+480 during the plateau of outburst confirmed the existence of the known 0.17085 . variations in the R-band with amplitude 0..06 and the 10-s QPOs, which are stronger in the I-band.

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978-94-010-3828-7Springer Science+Business Media New York 2001

Ballad

The 2000 April Multiwavelength Campaign of GRS 1915+105st campaigns ever made for this source covering the broad band from radio to .-rays. Multiwavelength light curves compiled from all the data reduced up to date and broad band spectra obtained with ASCA and RXTE are presented.

公理

Optical Observations of the X-Ray Transients XTE J1859 +226 and XTE J1118+480 Astronomical Observatory of Nikolaev State University. The observations of XTE J1859+226 were obtained in November 1999 and April 2000. The observations of the XTE Jl 118+480 started in April 2000. The light curves are presented here.

escalate

Recent Hubble Space Telescope Results on X-Ray Novaeirst outburst observations of X-ray novae with this instrument. We followed broad band spectral evolution, detected correlated X-ray/UV rapid variability and performed high resolution UV spectroscopy. We present a summary of initial results on the spectral energy distributions observed.

山崩

V404 CYG: 10 Years in Quiescenceh maxima and minima from year to year over 1992–2000. The most prominent are variations of the depth of minimum at phase 0.0 in V (1992–1997) and at phase 0.5 in R (1998–2000). The ∽ .-. QPOs persist but with variable amplitude.

lattice

Recent Results on X-Ray Novae and Microquasars at Radio and Infrared Wavelengthsnstance, radio interferometers are routinely the first ones to provide accurate subarcsec positions allowing further detailed studies. Similarly, infrared spectroscopy of highly obscured systems is the best way to unveil the often elusive nature of their companion star. In this talk I will review so

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