Open AccessJournal Article
LINE INTENSITIES AND MOLECULAR OPACITIES OF THE FeH F ^4Delta~i-X ^4Delta~i TRANSITION
C. W. Bauschlicher,M. Dulick +1 more
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This article is published in The Astrophysical Journal.The article was published on 2003-01-01 and is currently open access. It has received 41 citations till now. The article focuses on the topics: Line (formation).read more
Citations
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Journal ArticleDOI
New spectral types L and T
TL;DR: The establishment of new spectral classes cooler than type M has had a brief, yet already rich, history as discussed by the authors, with a flood of new discoveries occurring in the late 1990s with the advent of deep, large area, digital sky surveys.
Journal ArticleDOI
Line and Mean Opacities for Ultracool Dwarfs and Extrasolar Planets
TL;DR: In this paper, the authors present the detailed sources of molecular opacity data employed by their group for this application and present tables of Rosseland and Planck mean opacities, which are of use in some studies of the atmospheres, interiors, and evolution of planets and brown dwarfs.
Journal ArticleDOI
L and t dwarf models and the l to t transition
TL;DR: In this paper, a new series of L and T dwarf spectral and atmosphere models as a function of gravity and metallicity, spanning the Teff range from 2200 to 700 K, are presented.
Journal ArticleDOI
Gaseous mean opacities for giant planet and ultracool dwarf atmospheres over a range of metallicities and temperatures
Richard S. Freedman,Richard S. Freedman,Jacob Lustig-Yaeger,Jonathan J. Fortney,Roxana Lupu,Mark S. Marley,Katharina Lodders +6 more
TL;DR: In this article, the authors presented new calculations of Rosseland and Planck gaseous mean opacities relevant to the atmospheres of giant planets and ultracool dwarfs.
Journal ArticleDOI
The effective temperature scale of M dwarfs
A. S. Rajpurohit,Céline Reylé,F. Allard,Derek Homeier,M. Schultheis,M. Schultheis,Michael S. Bessell,Annie C. Robin +7 more
TL;DR: In this paper, the authors compare two samples of optical spectra covering the whole M dwarfs sequence with the most recent BT-Settl synthetic spectra and use a � 2 minimization technique to determine Teff.
References
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Journal ArticleDOI
New spectral types L and T
TL;DR: The establishment of new spectral classes cooler than type M has had a brief, yet already rich, history as discussed by the authors, with a flood of new discoveries occurring in the late 1990s with the advent of deep, large area, digital sky surveys.
Journal ArticleDOI
Line and Mean Opacities for Ultracool Dwarfs and Extrasolar Planets
TL;DR: In this paper, the authors present the detailed sources of molecular opacity data employed by their group for this application and present tables of Rosseland and Planck mean opacities, which are of use in some studies of the atmospheres, interiors, and evolution of planets and brown dwarfs.
Journal ArticleDOI
L and t dwarf models and the l to t transition
TL;DR: In this paper, a new series of L and T dwarf spectral and atmosphere models as a function of gravity and metallicity, spanning the Teff range from 2200 to 700 K, are presented.
Journal ArticleDOI
Atmospheric parameters of field l and t dwarfs
Michael C. Cushing,Michael C. Cushing,Mark S. Marley,Didier Saumon,Brandon C. Kelly,William D. Vacca,John Rayner,Richard S. Freedman,Katharina Lodders,Thomas L. Roellig +9 more
TL;DR: In this paper, an analysis of the 0.95-14.5?m spectral energy distributions of nine field ultracool dwarfs with spectral types ranging from L 1 to T 4.5 is presented.
Journal ArticleDOI
ExoMol: molecular line lists for exoplanet and other atmospheres
TL;DR: The ExoMol project as discussed by the authors provides spectroscopic data on all the molecular transitions of importance in the atmospheres of exoplanets, which can be used for studies on cool stars, brown dwarfs and circumstellar environments.