Response of Atmospheric Biomarkers to NO(x)-Induced Photochemistry Generated by Stellar Cosmic Rays for Earth-like Planets in the Habitable Zone of M Dwarf Stars

Understanding whether M dwarf stars may host habitable planets with Earth-like atmospheres and biospheres is a major goal in exoplanet research. If such planets exist, the question remains as to whether they could be identified via spectral signatures of biomarkers. Such planets may be exposed to ex...

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Détails bibliographiques
Auteurs principaux: Grenfell, John Lee, Grießmeier, Jean-Mathias, von Paris, Philip, Patzer, A. Beate C., Lammer, Helmut, Stracke, Barbara, Gebauer, Stefanie, Schreier, Franz, Rauer, Heike
Format: Artigo
Langue:Inglês
Publié: Mary Ann Liebert, Inc. 2012
Sujets:
Research Articles
Accès en ligne:https://ncbi.nlm.nih.gov/pmc/articles/PMC3522229/
https://ncbi.nlm.nih.gov/pubmed/23215581
https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1089/ast.2011.0682
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