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• W2117473902 abstract "We present a preliminary analysis of the 1-10 keV spectrum of the massive X-ray binary Cygnus X-3, obtained with the high-energy transmission grating spectrometer on the Chandra X-Ray Observatory. The source reveals a richly detailed discrete emission spectrum, with clear signatures of photoionization-driven excitation. Among the spectroscopic novelties in the data are the first astrophysical detections of a number of He-like triplets (Si, S, Ar) with emission-line ratios characteristic of photoionization equilibrium, fully resolved narrow radiative recombination continua of Mg, Si, and S, the presence of the H-like Fe Balmer series, and a clear detection of an approximately 800 km s-1 large-scale velocity field as well as an approximately 1500 km s-1 FWHM Doppler broadening in the source. We briefly touch on the implications of these findings for the structure of the Wolf-Rayet wind." @default.
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• W2117473902 date "2000-04-20" @default.
• W2117473902 modified "2023-10-13" @default.
• W2117473902 title "High-Resolution Spectroscopy of the X-Ray–photoionized Wind in Cygnus X-3 with the [ITAL]Chandra[/ITAL] High-Energy Transmission Grating Spectrometer" @default.
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• W2117473902 doi "https://doi.org/10.1086/312608" @default.
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