Radiative Transfer in Axial Symmetry

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$EinfÃ¼hrung in LATEX PD Dr. Thorsten Nagel - UniversitÃ¤t TÃ¼bingen$

$LaTeX Vorlesung - Typographie mit LaTeX -- Schriftarten und ...$

lower boundary condition
mean intensity rotation axis – the grid is defined by global properties – advantage – better description in outer regions, where the radiation field is strongly anisotropic
Page 1 and 2: Radiative Transfer in Axial Symmetr
Page 3 and 4: description of the method method pr
Page 5 and 6: longitudinal planes whole radiation
Page 7 and 8: integration I (B) = I (A) e −∆
Page 9: solution in the central region C
Page 13 and 14: parallelization - MPI - memory × c
Page 15 and 16: method applicability - limb darkeni
Page 18 and 19: stellar rotation - rapidly rotating
Page 20 and 21: stellar wind - optically thick atmo
Page 22 and 23: discs - protostellar discs - catacl
Page 24 and 25: choice of the systems - the quiesce
Page 26 and 27: SS Cyg - quiescent phase - Hα y [R
Page 28 and 29: SS Cyg - quiescent phase - Hγ y [R
Page 30 and 31: an AM CVn star - P orb < 1 hour =
Page 32 and 33: an AM CVn star - HeI 4923Å relativ
Page 34 and 35: Where it can play the role? - edge-

Radiative Transfer in Axial Symmetry

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