The DOI matches its Crossref record; 4 of the 4 references it cites were found in a registry or an index.
A Nongray Theory of Extrasolar Giant Planets and Brown Dwarfs
Open accessAbstract
We present the results of a new series of nongray calculations of the atmospheres, spectra, colors, and evolution of extrasolar giant planets (EGPs) and brown dwarfs for effective temperatures below 1300 K. This theory encompasses most of the mass/age parameter space occupied by substellar objects and is the first spectral study down to 100 K. These calculations are in aid of the multitude of searches being conducted or planned around the world for giant planets and brown dwarfs and reveal the exotic nature of the class. Generically, absorption by H 2 at longer wavelengths and H 2 O opacity windows at shorter wavelengths conspire to redistribute flux blueward. Below 1200 K, methane is the dominant carbon bearing molecule and is a universal diagnostic feature of EGP and brown dwarf spectra. We find that the primary bands in which to search are Z (~1.05 μm), J (~1.2 μm), H (~1.6 μm), K (~2.2 μm), M (~5 μm), and N (~10 μm), that enhancements of the emergent flux over blackbody values, in particular in the near infrared, can be by many orders of magnitude, and that the infrared colors of EGPs and brown dwarfs are much bluer than previously believed. In particular, relative to J and H , the K band flux is reduced by CH 4 and H 2 absorption. Furthermore, we conclude that for T eff 's below 1200 K most or all true metals may be sequestered below the photosphere, that an interior radiative zone is a generic feature of substellar objects, and that clouds of H 2 O and NH 3 are formed for T eff 's below ~400 and ~200 K, respectively. This study is done for solar-metallicity objects in isolation and does not include the effects of stellar insulation. Nevertheless, it is a comprehensive attempt to bridge the gap between the planetary and stellar realms and to develop a nongray theory of objects from 0.3 M J ("Saturn") to 70 M J (~0.07 M ☉ ). We find that the detection ranges for brown dwarf/EGP discovery of both ground- and space-based telescopes are larger than previously estimated.
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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
Search for Past Life on Mars: Possible Relic Biogenic Activity in Martian Meteorite ALH84001
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Ingersoll, A. P., & Pollard, D. (1982) · Icarus · doi:10.1016/0019-1035(82)90169-5 · Cited by 193
Cited by
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
Kirkpatrick, J. D., Reid, I. N., Liebert, J., Cutri, R. M., Nelson, B., Beichman, C. A., Dahn, C. C., Monet, D. G., Gizis, J. E., & Skrutskie, M. F. (1999) · The Astrophysical Journal · doi:10.1086/307414 · Cited by 992
Evolutionary models for cool brown dwarfs and extrasolar giant planets. The case of HD 209458
Baraffe, I., Chabrier, G., Barman, T., Allard, F. C., & Hauschildt, P. H. (2003) · Springer Link (Chiba Institute of Technology) · doi:10.1051/0004-6361:20030252/pdf · Cited by 916
The theory of brown dwarfs and extrasolar giant planets
Burrows, A., Hubbard, W. B., Lunine, J. I., & Liebert, J. (2001) · Reviews of Modern Physics · doi:10.1103/revmodphys.73.719 · Cited by 819
Self-citationThe 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
“…of isolated brown dwarfs—a relatively simple case of stellar evolution—has been studied extensively for the past 20 years and is well understood (D’Antona & Mazzitelli 1985; Nelson et al. 1986; Burrows et al. 1989, 1997; Burrows & Liebert 1993; Chabrier et al. 2000a, 2000b; Baraffe et al. 2002).”
BackgroundMethodInfluentialSelf-citation
Metadata
- Authors
- Burrows, A., Marley, M., Hubbard, W. B., Lunine, J. I., Guillot, T., Saumon, D., Freedman, R., Sudarsky, D., & Sharp, C.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 1997-12-20
- Volume
- 491
- Issue
- 2
- Pages
- 856-875
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W1985663566
- Cited by
- 1,390
- References
- 4
- FWCI
- 39.15
- Type
- journal article
- Language
- en
- Open access
- bronze
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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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