Fig. 7 from Chemical Abundances of the Secondary Star in the Black Hole X‐Ray Binary XTE J1118+480

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution

Export to PDF

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. 7.

Abundance ratios of the secondary star in XTE J1118+480 (large crosses) compared with the abundances of G and K metal‐rich dwarf stars. Galactic trends were taken from Gilli et al. (2006). The size of the cross indicates the uncertainty. Filled and empty circles correspond to abundances for exoplanet host stars and stars without known exoplanet companions, respectively. The dash‐dotted lines indicate solar abundance values.

Other Images in This Article

Copyright and Terms & Conditions