A Black Hole in the Superluminal Source SAX J1819.3-2525 (V4641 Sgr)

@article{Orosz2000ABH,
  title={A Black Hole in the Superluminal Source SAX J1819.3-2525 (V4641 Sgr)},
  author={J. Orosz and E. Kuulkers and M. V. D. Klis and J. Mcclintock and Michael R. Garcia Paul J. Callanan and C. Bailyn and R. Jain and R. Remillard},
  journal={International Journal of Std & Aids},
  year={2000}
}
  • J. Orosz, E. Kuulkers, +5 authors R. Remillard
  • Published 2000
  • Medicine, Physics, Sociology
  • International Journal of Std & Aids
  • Spectroscopic observations of the fast X-ray transient and superluminal jet source SAX J1819.3-2525 (V4641 Sgr) reveal a best-fitting period of Pspect = 2.81678 ± 0.00056 days and a semiamplitude of K2 = 211.0 ± 3.1 km s-1. The optical mass function is f(M) = 2.74 ± 0.12 M☉. We find a photometric period of Pphoto = 2.81730 ± 0.00001 days using a light curve measured from photographic plates. The folded light curve resembles an ellipsoidal light curve with two maxima of roughly equal height and… CONTINUE READING
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    References

    Publications referenced by this paper.
    SHOWING 1-10 OF 39 REFERENCES
    Orbital Parameters for the Soft X-Ray Transient 4U 1543–47: Evidence for a Black Hole
    • 82
    • PDF
    Optical Observations of GRO J1655?40 in Quiescence. I. A Precise Mass for the Black Hole Primary
    • 254
    • PDF
    Light Curves and Radio Structure of the 1999 September Transient Event in V4641 Sagittarii (=XTE J1819-254=SAX J1819.3-2525)
    • 78
    • Highly Influential
    • PDF
    Sources of Relativistic Jets in the Galaxy
    • 653
    • Highly Influential
    • PDF
    The observation and analysis of stellar photospheres
    • 1,880
    • Highly Influential
    • PDF
    A TiO study of the black hole binary GRO J0422+32 in a very low state
    • 34
    • PDF