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Investigating the High-energy Radiation Environment of Planets in Sun-like Binary Systems

  • Authors: Patrick R. Behr, Kevin France, Nicholas Kruczek, Nicholas Nell, Brian Fleming, Stefan Ulrich, Girish M. Duvvuri, Amy Louca, Yamila Miguel

Patrick R. Behr et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 6.

Stellar SEDs for α Cen A (blue) and B (orange) binned to 1 Å. The SED of the Sun, scaled to a distance of 1.33 pc, from T. N. Woods et al. (2009) is shown in gray for comparison. Colored background regions show the various regions described in Section 5.2. The regions containing the reconstructed Lyα (1214–1217 Å, Section 5.2.4) and SISTINE detector gap (1270–1300 Å, Section 5.2.3) are not colored for clarity. The PHOENIX model extends to 107 Å but we have restricted the y-axis to 10−17 erg s−1 cm−2 Å−1, again to aid visual clarity of features within the main spectra.

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