The DOI matches its Crossref record; 45 of the 45 references it cites were found in a registry or an index.
A correlation between the heavy element content of transiting extrasolar planets and the metallicity of their parent stars
Open accessAbstract
Context.Nine extrasolar planets with masses between 110 and 430 are known to transit their star. The knowledge of their masses and radii allows an estimate of their composition, but uncertainties on equations of state, opacities and possible missing energy sources imply that only inaccurate constraints can be derived when considering each planet separately.
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Cites
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The Limiting Effects of Dust in Brown Dwarf Model Atmospheres
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Self-citationAnnual Review of Earth and Planetary Sciences
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Alibert, Y., Mordasini, C., Benz, W., & Winisdoerffer, C. (2005) · Astronomy & Astrophysics · doi:10.1051/0004-6361:20042032 · Cited by 685
Atmospheric circulation and tides of “51 Pegasus b-like” planets
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Self-citationInfrared radiation from an extrasolar planet
Deming, D., Seager, S., Richardson, L. J., & Harrington, J. (2005) · Nature · doi:10.1038/nature03507 · Cited by 614
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The interiors of giant planets: Models and outstanding questions.
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Self-citationBouchy, F., Udry, S., Mayor, M., Moutou, C., Pont, F., Iribarne, N., Da Silva, R., Ilovaisky, S., Queloz, D., Santos, N. C., et al. (2005) · Astronomy & Astrophysics · doi:10.1051/0004-6361:200500201 · Cited by 495
Self-citation
Cited by
SPECTRAL AND PHOTOMETRIC DIAGNOSTICS OF GIANT PLANET FORMATION SCENARIOS
Spiegel, D. S., & Burrows, A. (2012) · The Astrophysical Journal · doi:10.1088/0004-637x/745/2/174 · Cited by 398
THE COMPOSITIONAL DIVERSITY OF EXTRASOLAR TERRESTRIAL PLANETS. I. IN SITU SIMULATIONS
Bond, J. C., O'Brien, D. P., & Lauretta, D. S. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/715/2/1050 · Cited by 308
WASP-1b and WASP-2b: two new transiting exoplanets detected with SuperWASP and SOPHIE
Cameron, A. C., Bouchy, F., Hebrard, G., Maxted, P., Pollacco, D., Pont, F., Skillen, I., Smalley, B., Street, R. A., West, R. G., et al. (2007) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2006.11350.x · Cited by 292
Self-citationWASP-17b: AN ULTRA-LOW DENSITY PLANET IN A PROBABLE RETROGRADE ORBIT
Anderson, D. R., Hellier, C., Gillon, M., Triaud, A. H. M. J., Smalley, B., Hebb, L., Cameron, A. C., Maxted, P. F. L., Queloz, D., West, R. G., et al. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/709/1/159 · Cited by 208
Metadata
- Authors
- Guillot, T., Santos, N. C., Pont, F., Iro, N., Melo, C., & Ribas, I.
- Venue
- Astronomy & Astrophysics
- Publisher
- EDP Sciences
- Published
- 2006-06-16
- Volume
- 453
- Issue
- 2
- Pages
- L21-L24
- ISSN
- 0004-6361 (ISSN-L)
- 1432-0746
- OpenAlex
- W2045315671
- Cited by
- 323
- References
- 45
- FWCI
- 17.93
- Type
- journal article
- Language
- en
- Open access
- bronze
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- Guillot, T., Santos, N. C., Pont, F., Iro, N., Melo, C., & Ribas, I. (2006). A correlation between the heavy element content of transiting extrasolar planets and the metallicity of their parent stars. Astronomy & Astrophysics. https://doi.org/10.1051/0004-6361%3A20065476
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Bibliographic data: Semantic Scholar, OpenAlex, Crossref.
Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.