CI Cam: Observations of the Dust Envelope Diameter
We spatially resolved the symbiotic star CI Cam, about 6 months after its April 1998 outburst, using the IOTA stellar interferometer. We measured the diameter...
CI non LTE spectral line formation in late-type stars
We present non-Local Thermodynamic Equilibrium (non-LTE) calculations for neutral carbon spectral line formation, carried out for a grid of model atmospheres...
Ci Non-LTE Spectral Line Formation in Late-Type Stars
We present the results from our non-LTE investigation for neutral carbon, which was carried out to remove potential systematic errors in stellar abundance...