Analysis of the profiles of strong lines in three F and G subdwarfs.
F and G subdwarf strong line profiles, discussing convection in calculating model atmosphere and resonance damping in hydrogen line profile
Swamy, K. S. K.↗
Engineering topics
Swamy, K. S. K.
Publications and source records attributed to Swamy, K. S. K..
Interstellar extinction by quartz grains.
Interstellar extinction cross sections calculated for quartz particles, results indicate quartz is not appreciable component of interstellar grains
Swamy, K. S. K.↗
Thermal emission by particles in NGC 7027.
IR continuum in planetary nebula NGC 7027 in terms of thermal emission by particles within nebula
Odell, C. R.↗
Damping constant of Fraunhofer lines.
Solar photosphere collisional damping by hydrogen atoms larger than electron damping for Fraunhofer lines
Swamy, K. S. K.↗
On the temperature of interstellar grains.
Temperatures of grain models using interstellar radiation field in solar neighborhood and optical data for graphite and ice
Swamy, K. S. K.↗
Unified model for interstellar extinction and polarization.
Interstellar polarization with graphite grains covered with dirty ice mantles matched with entire range of observed interstellar extinction
POLARIZATION↗