Line Formation in CH Cyg: A Symbiotic Binary

Details Line Formation in CH Cyg: A Symbiotic Binary Line Formation in CH Cyg: A Symbiotic Binary

Dec 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996rmxac...5..111b&link_type=abstract

Workshop on Colliding Winds in Binary Stars to Honor Jorge Sahade, vol. 5, p. 111

Computer Science

Symbiotic Stars, Temperature, Excitation, Iron Isotopes, Estimating, Dimensions, Binary Data, Cygnus Constellation, Self Absorption, Formations, Fracturing

Scientific paper

Applying the Self Absorption Curve (SAC) method to the symbiotic binary CH Cyg, we determine the excitation temperature of the (Fe II) line formation region and that of the permitted Fe II lines. We estimate the dimensions of the Fe II line formation regions, and we conclude that these lines can form in a region of the wind starting to fall towards the hot component.

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