Fig. 4 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. 4.

Best synthetic spectral fits to the Keck ESI spectrum of the secondary star in the XTE J1118+480 system (bottom), and the same for a template star (properly broadened) shown for comparison (top). Synthetic spectra are computed for solar abundances (dashed line) and best‐fit abundances (solid lines).

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