Orbital Parameters for the Black Hole Binary XTE J1650–500*

@article{Orosz2004OrbitalPF,
  title={Orbital Parameters for the Black Hole Binary XTE J1650–500*},
  author={J. Orosz and J. Mcclintock and R. Remillard and S. Corbel},
  journal={The Astrophysical Journal},
  year={2004},
  volume={616},
  pages={376-382}
}
  • J. Orosz, J. Mcclintock, +1 author S. Corbel
  • Published 2004
  • Physics
  • The Astrophysical Journal
  • We present R-band photometry of the X-ray transient and candidate black hole binary XTE J1650-500 obtained between 2003 May and August with the 6.5 m Clay telescope. A timing analysis of these data reveals a photometric period of 0.3205 ± 0.0007 days (i.e., 7.63 hr) with a possible alias at 0.3785 days (9.12 hr). Our photometry completely rules out the previously published spectroscopic period of 0.212 days (5.09 hr). Consequently, we reanalyzed the 15 archival ESO VLT spectra (obtained 2002… CONTINUE READING
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    References

    SHOWING 1-10 OF 48 REFERENCES
    Optical Outburst of the Halo Black Hole X-ray Transient XTE J1118+480
    • 91
    • PDF
    Dynamical Evidence for a Black Hole in the Microquasar XTE J1550-564
    • 185
    • PDF
    A Black Hole in the Superluminal Source SAX J1819.3-2525 (V4641 Sgr)
    • 163
    • PDF
    GRO J0422+32: The Lowest Mass Black Hole?*
    • 63
    • PDF