The DOI matches its Crossref record; 3 of the 3 references it cites were found in a registry or an index.
A chemical model for the atmosphere of hot Jupiters
Open accessAbstract
Context. The atmosphere of hot Jupiters can be probed by primary transit and secondary eclipse spectroscopy. Owing to the intense UV irradiation, mixing, and circulation, their chemical composition is maintained out of equilibrium and must be modeled with kinetic models.
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Cites
Detection of Planetary Transits Across a Sun-like Star
Charbonneau, D., Brown, T. M., Latham, D. W., & Mayor, M. (2000) · The Astrophysical Journal · doi:10.1086/312457 · Cited by 1,415
The Occurrence and Mass Distribution of Close-in Super-Earths, Neptunes, and Jupiters
Howard, A. W., Marcy, G. W., Johnson, J. A., Fischer, D. A., Wright, J. T., Isaacson, H., Valenti, J. A., Anderson, J., Lin, D. N. C., & Ida, S. (2010) · Science · doi:10.1126/science.1194854 · Cited by 635
Planetary Candidates Observed by Kepler, III: Analysis of the First 16 Months of Data
Batalha, N. M., Rowe, J. F., Bryson, S. T., Barclay, T., Burke, C. J., Caldwell, D. A., Christiansen, J. L., Mullally, F., Thompson, S. E., Brown, T. M., et al. (2012) · arXiv · doi:10.48550/arxiv.1202.5852 · Cited by 10
Cited by
A chemical survey of exoplanets with ARIEL
Tinetti, G., Drossart, P., Eccleston, P., Hartogh, P., Heske, A., Leconte, J., Micela, G., Ollivier, M., Pilbratt, G., Puig, L., et al. (2018) · Experimental Astronomy · doi:10.1007/s10686-018-9598-x · Cited by 445
Self-citationExoMol line lists – III. An improved hot rotation-vibration line list for HCN and HNC
Barber, R. J., Strange, J. K., Hill, C., Polyansky, O. L., Mellau, G. C., Yurchenko, S. N., & Tennyson, J. (2014) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stt2011 · Cited by 323
COMPOSITIONAL DIVERSITY IN THE ATMOSPHERES OF HOT NEPTUNES, WITH APPLICATION TO GJ 436b
Moses, J. I., Line, M. R., Visscher, C., Richardson, M. R., Nettelmann, N., Fortney, J. J., Barman, T. S., Stevenson, K. B., & Madhusudhan, N. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/777/1/34 · Cited by 299
Atmospheric nitrogen evolution on Earth and Venus
Wordsworth, R. D. (2016) · Earth and Planetary Science Letters · doi:10.1016/j.epsl.2016.04.002 · Cited by 78
Metadata
- Authors
- Venot, O., Hébrard, E., Agúndez, M., Dobrijevic, M., Selsis, F., Hersant, F., Iro, N., & Bounaceur, R.
- Venue
- Astronomy & Astrophysics
- Publisher
- EDP Sciences
- Published
- 2012-10
- Volume
- 546
- Pages
- A43
- ISSN
- 0004-6361 (ISSN-L)
- 1432-0746
- OpenAlex
- W2124216665
- Cited by
- 255
- References
- 3
- FWCI
- 8.15
- Type
- journal article
- Language
- en
- Open access
- bronze
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- Venot, O., Hébrard, E., Agúndez, M., Dobrijevic, M., Selsis, F., Hersant, F., Iro, N., & Bounaceur, R. (2012). A chemical model for the atmosphere of hot Jupiters. Astronomy & Astrophysics. https://doi.org/10.1051/0004-6361/201219310
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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
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