Hostname: page-component-76fb5796d-wq484 Total loading time: 0 Render date: 2024-04-26T09:00:28.274Z Has data issue: false hasContentIssue false
  • English
  • Français

Reconstructing the Stellar UV and EUV Emission that Controls the Chemistry of Exoplanet Atmospheres

Published online by Cambridge University Press:  29 April 2014

Jeffrey L. Linsky ,
Kevin France  and
Tom Ayres
Jeffrey L. Linsky
Affiliation:
JILA, University of Colorado and NIST, Boulder CO 80309-0440, USA email: jlinsky@jila.colorado.edu
Kevin France
Affiliation:
CASA, University of Colorado, Boulder CO 80309-0389, USA
Tom Ayres
Affiliation:
CASA, University of Colorado, Boulder CO 80309-0389, USA
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Lyman-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.

Keywords

exoplanet atmospheresultraviolet stellar spectraextreme ultraviolet stellar spectrahydrogen Lyman-α emission
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S293: Formation, Detection, and Characterization of Extrasolar Habitable Planets , August 2012 , pp. 309 - 314
Copyright
Copyright © International Astronomical Union 2014 

References

Avrett, E. H. & Loeser, R. 2008, ApJS, 175, 229Google Scholar
Fontenla, J. M., Harder, J., Livingston, W., Snow, M., & Woods, T. 2011, JGR, 116, D20108CrossRefGoogle Scholar
France, K., Linsky, J. L., Feng, T., Froning, C. S., & Roberge, A. 2012, ApJ, 750, 32Google Scholar
France, K., et al. 2013, ApJ 763 article id.149Google Scholar
Kopparapu, R. K., Kasting, J. E., & Zahnle, K. J. 2012, ApJ, 745, 77Google Scholar
Linsky, J. L., France, K, & Ayres, T. 2013, ApJ 766 article id.69Google Scholar
Murray-Clay, R. A., Chiang, E. I., & Murray, N. 2009 ApJ, 693, 23Google Scholar
Ribas, I., Guinan, E. F., Güdel, M., & Audard, M. 2005, ApJ, 622, 680CrossRefGoogle Scholar
Ribas, I., Porto de Mello, G. F., Ferreira, L. D., Hébrard, E., Selsis, F., Catalán, S., Garcés, A., do Nascimento, J. D. Jr., & de Medeiros, J. R. 2010, ApJ, 714, 384Google Scholar
Snow, M., McClintock, W. E., Rottman, G., & Woods, T. N. 2005, Solar Phys., 230, 295Google Scholar
Wood, B. E., Redfield, S., Linsky, J. L., Müller, H.-R., & Zank, G. P. 2005, ApJS, 159, 118Google Scholar
Woods, T. N., et al. 2009, J. Geophys. Res., 36, L01101Google Scholar