The High-Resolution X-Ray Spectrum of SS 433 Using the Chandra HETGS

We present observations of SS 433 using the Chandra High Energy Transmission Grating Spectrometer. Many emission lines of highly ionized elements are detected with relativistic blue and red Doppler shifts. The lines are measurably broadened to 1700 km s[superscript -1] (FWHM), and the widths do not...

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Bibliographic Details
Main Authors: Canizares, Claude R., Schulz, Norbert S., Marshall, Herman
Other Authors: MIT Kavli Institute for Astrophysics and Space Research
Format: Article
Language:en_US
Published: IOP Publishing 2013
Online Access:http://hdl.handle.net/1721.1/76232
https://orcid.org/0000-0002-5769-8441