Radiative Transfer with Opacity Distribution Functions: Application to Narrowband Filters

Modeling of stellar radiative intensities in various spectral passbands plays an important role in stellar physics. At the same time, direct calculation of the high-resolution spectrum and then integration of it over the given spectral passband is computationally demanding due to the vast number of...

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Veröffentlicht in:	The Astrophysical journal. Supplement series 2021-07, Vol.255 (1), p.3
Hauptverfasser:	Anusha, L. S., Shapiro, A. I., Witzke, V., Cernetic, M., Solanki, S. K., Gizon, L.
Format:	Artikel
Sprache:	eng
Schlagworte:	Approximation Astronomical models Atmosphere Atmospheric models Atomic properties Computational fluid dynamics Cubes Distribution functions Exoplanet astronomy Filters Magnetohydrodynamics Mathematical analysis Narrowband Opacity Physics Radiative transfer Radiative transfer equation Spectra Stellar atmospheres Stellar atmospheric opacity Stellar models Stellar physics Three dimensional models
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