Carbon Monoxide and the Potential for Prebiotic Chemistry on Habitable Planets around Main Sequence M Stars-Reference-Cited by-同舟云学术

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Carbon Monoxide and the Potential for Prebiotic Chemistry on Habitable Planets around Main Sequence M Stars

Published:2016-10 Issue:10 Volume:16 Page:744-754
ISSN:1531-1074
Container-title:Astrobiology
language:en
Short-container-title:Astrobiology

Author:

Nava-Sedeño J. Manik¹,Ortiz-Cervantes Adrian²,Segura Antígona³,Domagal-Goldman Shawn D.⁴

Affiliation:

1. Department for Innovative Methods of Computing, ZIH, Technische Universität Dresden, Dresden, Germany.

2. Structural Bioinformatics and Computational Biology, BIOTEC, Technische Universität Dresden, Dresden, Germany.

3. Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de México, México D.F., México.

4. Planetary Environments Laboratory, NASA Goddard Space Flight Center, Greenbelt, Maryland, USA.

Publisher

Mary Ann Liebert Inc

Subject

Space and Planetary Science,Agricultural and Biological Sciences (miscellaneous)

Link

http://www.liebertpub.com/doi/pdf/10.1089/ast.2015.1435

Reference46 articles.

1. New insights into prebiotic chemistry from Stanley Miller's spark discharge experiments

2. Properties of solar X-ray flares and proton event forecasting

3. Proton Events and X-ray Flares in the Last Three Solar Cycles

4. Peak-Size Distributions of Proton Fluxes and Associated Soft X-Ray Flares

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