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Sara Seager of the Massachusetts Institute of Technology noted that Dr. Kaltenegger's model atmospheres were limited to water, carbon dioxide and nitrogen, like the Earth.
In addition, we constructed a new generation of metal line-blanketed non-LTE model atmospheres for NSs.
The observed monthly mean temperature profiles are compared with different model atmospheres (CIRA-86 and MSISE-90).
We present calculations of LTE model atmospheres of some ring on the accretion disk, which are illuminated by isotropic hard X-rays.
The CS bands and the band heads of the CO fundamental bands are weaker in the observed spectra than in the ones predicted by our model atmospheres.
The spectral shape of the radiation emitted by Population III stars on the main sequence may be derived by combining stellar structure calculations with detailed LTE and non-LTE model atmospheres (Cojazzi et al. 2000; Tumlinson and Shull 2000; Bromm et al. 2001b; Schaerer 2002, 2003).
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We discuss model atmosphere fits.
The sensitivity of the simulations to the equivalent depth of the model atmosphere was tested.
The model atmosphere extended from the surface to 70 km and had the starting composition, pressure and temperature of the 1976 US Standard Atmosphere.
The initial thermodynamic structure of the unperturbed model atmosphere is defined by moist adiabatic lapse rate up to 17 km and a constant temperature above this height.
In order to suppress the frequency variation to enable narrowband filtering, a predicted Doppler frequency based on a model atmosphere is subtracted from the original signal by heterodyning.
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