Thermal emission by grains and the free-free emission from planetary nebulae.
Thermal and free-free emission from planetary nebulae based on graphite grain model, discussing IR fluxes
Krishna Swamy, K. S.↗
Engineering topics
Krishna Swamy, K. S.
Publications and source records attributed to Krishna Swamy, K. S..
A spectral feature of grains at 10 mu?
Late type stars with emission peak wavelength approximating graphite Debye frequency induced by graphite impurity atoms
Krishna Swamy, K. S.↗
Strengths of the fundamental bands of ice and solid hydrogen in composite grains.
Extinction efficiency of graphite core interstellar grains with solid hydrogen and ice mantles, using theoretical models
Krishna Swamy, K. S.↗
Atmospheres of metal-deficient stars - Main sequence stars.
Atmospheric models for metal deficient stars of K and G spectral type, studying reduced metal abundance effect on atmospheric structure
Krishna Swamy, K. S.↗
Extinction by interstellar grains, Mie particles and polycyclic aromatic molecules.
Interstellar extinction models of classical Mie particles and quantum mechanical polycyclic aromatic molecules
Donn, B.↗
Inversion of density in the convective zone.
Density inversion in convective zone of stellar photospheres occurring in Eridani atmospheric model under certain conditions
Krishna Swamy, K. S.↗
Comparison of the convective model atmospheres of epsilon Eridani and GMB 1830.
Model atmospheres for epsilon Eridani and GMB 1830 computed using mixing-length theory in convective zone to compare atmospheres for differences caused by metal deficiency stars
Krishna Swamy, K. S.↗