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Orbital Parameters for the Black Hole Binary XTE J1650−500

  • Authors: Jerome A. Orosz, Jeffrey E. McClintock, Ronald A. Remillard, and Stéphane Corbel

Orosz et al. 2004 The Astrophysical Journal 616 376.

  • Provider: AAS Journals

Caption: Fig. 5.

Bottom panel: Best normalized rest‐frame spectrum of J1650 (top spectrum), normalized spectrum of the K4 V star BS 5568 scaled by 0.1 and shifted upward by 0.5 (bottom spectrum), and difference spectrum (middle spectrum). Top panel: Cross‐correlation function of the best rest‐frame spectrum against the K4 V star BS 5568.

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