A Possible Bifurcation in Atmospheres of Strongly Irradiated Stars and Planets
暂无分享,去创建一个
I. Hubeny | A. Burrows | A. Burrows | D. Sudarsky | I. Hubeny | D. Sudarsky
[1] R. S. Ram,et al. New CrH Opacities for the Study of L and Brown Dwarf Atmospheres , 2002, astro-ph/0206159.
[2] A. Borysow,et al. Collision-induced absorption coefficients of H2 pairs at temperatures from 60 K to 1000 K , 2002 .
[3] Laurence S. Rothman,et al. Reprint of: The HITRAN molecular spectroscopic database and HAWKS (HITRAN Atmospheric Workstation): 1996 edition , 1998 .
[4] Ivan Hubeny,et al. A computer program for calculating non-LTE model stellar atmospheres , 1988 .
[5] K. Strong,et al. Spectral parameters of self- and hydrogen-broadened methane from 2000 to 9500 cm-1 for remote sounding of the atmosphere of jupiter , 1993 .
[6] B. Fegley,et al. Atmospheric Chemistry in Giant Planets, Brown Dwarfs, and Low-Mass Dwarf Stars: I. Carbon, Nitrogen, and Oxygen , 2002 .
[7] Lothar Frommhold,et al. A new computation of the infrared absorption by H2 pairs in the fundamental band at temperatures from 600 to 5000 K , 1990 .
[8] Adam Burrows,et al. The Near-Infrared and Optical Spectra of Methane Dwarfs and Brown Dwarfs , 1999, astro-ph/9908078.
[9] E. Karkoschka. Spectrophotometry of the Jovian Planets and Titan at 300- to 1000-nm Wavelength: The Methane Spectrum , 1994 .
[10] Saurabh Jha,et al. An extrasolar planet that transits the disk of its parent star , 2003, Nature.
[11] J. Lunine,et al. Some constraints on a greenhouse atmosphere for Triton , 1988 .
[12] A. Burrows,et al. Chemical Equilibrium Abundances in Brown Dwarf and Extrasolar Giant Planet Atmospheres , 1999 .
[13] L. Rothman,et al. Direct numerical diagonalization: Wave of the future , 1992 .
[14] D. G. Hummer. The effect of reflected and external radiation on stellar flux distributions , 1982 .
[15] S. Mahulikar,et al. Physica Scripta , 2004 .
[16] Noelle A. Scott,et al. Management and study of spectroscopic information: The GEISA program , 1992 .
[17] Adam Burrows,et al. Theoretical Spectra and Atmospheres of Extrasolar Giant Planets , 2003 .
[18] Harry Partridge,et al. The determination of an accurate isotope dependent potential energy surface for water from extensive ab initio calculations and experimental data , 1997 .
[19] Peter H. Hauschildt,et al. TiO and H2O Absorption Lines in Cool Stellar Atmospheres , 2000, astro-ph/0008465.
[20] I. Hubeny. Vertical structure of accretion disks: A simplified analytical model , 1990 .
[21] A. Borysow,et al. Modeling of Collision-Induced Infrared Absorption Spectra of H2 Pairs in the First Overtone Band at Temperatures from 20 to 500 K , 1995 .
[22] Jean-Paul Champion,et al. T.D.S. spectroscopic databank for spherical tops: DOS version , 1994 .
[23] V. A. Sinel’shchikov,et al. Collisional Broadening of the Na-D Lines by Molecular Gases , 1999 .
[24] D. Goorvitch. Infrared CO line for the X 1 Sigma(+) state , 1994 .
[25] Calculation of spectroscopic parameters for diatomic molecules of atmospheric interest , 1990 .
[26] Ivan Hubeny,et al. Non-LTE line-blanketed model atmospheres of hot stars. 1: Hybrid complete linearization/accelerated lambda iteration method , 1995 .
[27] B. Pagel,et al. Stellar atmospheres , 1978, Nature.
[28] V. M. Devi,et al. THE HITRAN MOLECULAR DATABASE: EDITIONS OF 1991 AND 1992 , 1992 .