Doppler modulation of hydrogen-like iron emission from Cygnus X-3

Details Doppler modulation of hydrogen-like iron emission from Cygnus X-3 Doppler modulation of hydrogen-like iron emission from Cygnus X-3

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aas...207.1110k&link_type=abstract

American Astronomical Society Meeting 207, #11.10; Bulletin of the American Astronomical Society, Vol. 37, p.1170

Astronomy and Astrophysics

Astronomy

Scientific paper

In previous work we studied the Doppler modulation of various emission lines in the X-rays from Cygnus X-3. This analysis revealed an interesting ionization structure in the stellar wind of this source. We extend this analysis with additional data and focus on the study of Fe XXV lines which should reveal the location the most intense phtoionization of the wind, presumably near the X-ray source.

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