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

AAS 207th Meeting, 8-12 January 2006
Session 11 Binary Models and Parameters
Poster, Monday, 9:20am-7:00pm, January 9, 2006, Exhibit Hall

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

M.C. Kaczmarczik, M.J. Stark (Lafayette College)

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.

If you would like more information about this abstract, please follow the link to http://www.lafayette.edu/~starkm/pub/aas-207-mike.html. This link was provided by the author. When you follow it, you will leave the Web site for this meeting; to return, you should use the Back comand on your browser.

The author(s) of this abstract have provided an email address for comments about the abstract: kaczmarm@lafayette.edu

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