Fig. 1 from Chemical Abundances of the Secondary Star in the Black Hole X‐Ray Binary XTE J1118+480

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Chemical Abundances of the Secondary Star in the Black Hole X‐Ray Binary XTE J1118+480

Authors: Jonay I. González Hernández, Rafael Rebolo, Garik Israelian, Alexei V. Filippenko, Ryan Chornock, Nozomu Tominaga, Hideyuki Umeda, and Ken'ichi Nomoto

González Hernández et al. 2008 The Astrophysical Journal 679 732.

Provider: AAS Journals

Caption: Fig. 1.

Radial velocities of XTE J1118+480 folded on the orbital solution of the data, together with the best‐fitting sinusoid. Individual velocity uncertainties are ≤7 km s⁻¹ and are not plotted, because they are always smaller than the symbol size. The bottom panel shows the residuals of the fit.

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