VUV-absorption cross section of CO2 at high temperatures and impact on exoplanet atmospheres
Ultraviolet (UV) absorption cross sections are an essential ingredient of photochemical atmosphere models. Exoplanet searches have unveiled a large population of short-period objects with hot atmospheres, very different from what we find in our solar system. Transiting exoplanets whose atmospheres...
| Main Authors: | , , , , , , , , |
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| Format: | Article |
| Language: | English |
| Published: |
EDP Sciences
2014-02-01
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| Series: | BIO Web of Conferences |
| Online Access: | http://dx.doi.org/10.1051/bioconf/20140201002 |