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ASTRONOMY & ASTROPHYSICS, ISSN 1432-0746, 05/2019, Volume 625, p. A107
Context. The study of exoplanetary atmospheres is key to understanding the differences between their physical, chemical, and dynamical processes. Until now,... 
COLLISION-INDUCED ABSORPTION | planets and satellites: atmospheres | STARLIGHT | METHANE | techniques: spectroscopic | ASTRONOMY & ASTROPHYSICS | MASS | PLANET | H-2 PAIRS | UPPER LIMIT | ORBITAL MOTION | planets and satellites: fundamental parameters
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2017, Volume 464, Issue 4, pp. 4247 - 4254
Journal Article
Journal Article
Astrophysical Journal, Supplement Series, ISSN 0067-0049, 01/2014, Volume 210, Issue 1, pp. 13 - 8
Journal Article
1983, Monographs on astronomical subjects, ISBN 0852743858, Volume 9, xv, 239
Book
Science, ISSN 0036-8075, 12/2018, Volume 362, Issue 6421, pp. 1360 - 1361
The atmospheres of planets orbiting other stars (exoplanets) are windows into their chemical composition and physical properties. For a planet that orbits... 
MULTIDISCIPLINARY SCIENCES | Near infrared radiation | Planetary atmospheres | Organic chemistry | Stellar atmospheres | Spectral resolution | Extrasolar planets | Atmosphere | Radiation | Irradiation | Chemical composition | Helium | Physical properties
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 02/2019, Volume 622
Context. Understanding of clouds is instrumental in interpreting current and future spectroscopic observations of exoplanets. Modeling clouds consistently is... 
Planetary atmospheres | Particle size | Nucleation | Clouds | Atmospheric models | Coagulation | Condensation | Optimization | Dependence | Cloud formation | Cloud thickness | Grain size | Spectroscopy | Parameters | Computer simulation | Extrasolar planets | Spectra | Sedimentation | Extrasolar giant planets | Thickness | Organic chemistry | Jupiter | Atmosphere | Particle transport | Astrochemistry | Transport | Computing time
Journal Article
Astronomy & astrophysics, ISSN 0004-6361, 05/2009, Volume 498, Issue 3, pp. 877 - 884
Context. In recent years, the solar chemical abundances have been studied in considerable detail because of discrepant values of solar metallicity inferred... 
Sun: abundances | hydrodynamics | GRANULATION | stars: abundances | OXYGEN | HYDROGEN | ELEMENTS | line: formation | HELIOSEISMOLOGY | STATISTICAL EQUILIBRIUM | SPECTRUM | SEPARATION RATIOS | DEGREE P-MODES | LINE FORMATION | ASTRONOMY & ASTROPHYSICS | Physics - Solar and Stellar Astrophysics
Journal Article