The DOI matches its Crossref record; 4 of the 4 references it cites were found in a registry or an index.
Evolutionary models for cool brown dwarfs and extrasolar giant planets. The case of HD 209458
Open accessAbstract
We present evolutionary models for cool brown dwarfs and extra-solar giant planets. The models reproduce the main trends of observed methane dwarfs in near-IR color-magnitude diagrams. We also present evolutionary models for irradiated planets, coupling for the first time irradiated atmosphere profiles and inner structures. We focus on HD 209458-like systems and show that irradiation effects can substantially affect the radius of sub-jovian mass giant planets. Irradiation effects, however, cannot alone explain the large observed radius of HD 209458b. Adopting assumptions which optimise irradiation effects and taking into account the extension of the outer atmospheric layers, we still find ~20% discrepancy between observed and theoretical radii. An extra source of energy seems to be required to explain the observed value of the first transit planet.
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Cites
A Jupiter-mass companion to a solar-type star
Mayor, M., & Queloz, D. (1995) · Nature · doi:10.1038/378355a0 · Cited by 4,111
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 Limiting Effects of Dust in Brown Dwarf Model Atmospheres
Allard, F., Hauschildt, P. H., Alexander, D. R., Tamanai, A., & Schweitzer, A. (2001) · The Astrophysical Journal · doi:10.1086/321547 · Cited by 1,062
Self-citationEvolution of “51 Pegasus b-like” planets
Guillot, T., & Showman, A. P. (2002) · Astronomy & Astrophysics · doi:10.1051/0004-6361:20011624 · Cited by 386
Cited by
MESA ISOCHRONES AND STELLAR TRACKS (MIST). I. SOLAR-SCALED MODELS
Choi, J., Dotter, A., Conroy, C., Cantiello, M., Paxton, B., & Johnson, B. D. (2016) · The Astrophysical Journal · doi:10.3847/0004-637x/823/2/102 · Cited by 2,922
Angular Differential Imaging: A Powerful High‐Contrast Imaging Technique
Marois, C., Lafreniere, D., Doyon, R., Macintosh, B., & Nadeau, D. (2006) · The Astrophysical Journal · doi:10.1086/500401 · Cited by 1,015
The Evolution of L and T Dwarfs in Color‐Magnitude Diagrams
Saumon, D., & Marley, M. S. (2008) · The Astrophysical Journal · doi:10.1086/592734 · Cited by 693
“Figures 2 and 3 compare our cloudless sequence with the COND03models of Baraffe et al. (2003) and our cloudy fsed ¼ 2 sequence with the DUSTY00 models of Chabrier et al. (2000b) and Baraffe et al. (2002), respectively.”
BackgroundMethodInfluentialOn the radiative equilibrium of irradiated planetary atmospheres
Guillot, T. (2010) · Astronomy and Astrophysics · doi:10.1051/0004-6361/200913396 · Cited by 573
Kirkpatrick, J. D. (2005) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.42.053102.134017 · Cited by 560
Metadata
- Authors
- Baraffe, I., Chabrier, G., Barman, T. S., Allard, F., & Hauschildt, P. H.
- Venue
- Astronomy & Astrophysics
- Publisher
- EDP Sciences
- Published
- 2003-04-14
- Volume
- 402
- Issue
- 2
- Pages
- 701-712
- ISSN
- 0004-6361 (ISSN-L)
- 1432-0746
- OpenAlex
- W1968690455
- Cited by
- 1,566
- References
- 4
- FWCI
- 33.64
- Type
- journal article
- Language
- en
- Open access
- bronze
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