Reconstructing the Stellar UV and EUV Emission that Controls the Chemistry of Exoplanet Atmospheres Conference Proceeding uri icon



  • AbstractLyman-α and extreme-ultraviolet radiation from exoplanet host stars are critically important for evaluating the phototchemistry of planetary atmospheres, but these emissions are largely or completely absorbed by hydrogen in the interstellar medium. We describe a new technique for estimating the intrinsic Lyman-α and EUV fluxes of F, G, K, and M stars using correlations with observable emission lines.

publication date

  • August 1, 2012

has restriction

  • bronze

Date in CU Experts

  • November 11, 2015 3:11 AM

Full Author List

  • Linsky JL; France K; Ayres T

author count

  • 3

Other Profiles

International Standard Serial Number (ISSN)

  • 1743-9213

Electronic International Standard Serial Number (EISSN)

  • 1743-9221

Additional Document Info

start page

  • 309

end page

  • 314


  • 8


  • S293