Accretion disc winds are a common, perhaps ubiquitous, feature of X-ray binaries, observed across multiple wavelengths and linked to disc atmospheres, jets and varying accretion states.
Erratum: ASCA Observations of the Absorption-Line Features from the Super-Luminal Jet Source GRS 1915+105
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We have discovered errors in the calculation of some of the Einstein coefficients in Table 5 and some plots in Figure 3. Due to the errors, the square-root section of the curves of growth of Fe xxvi Ka and Kb, and Ni xxviii Ka in Figure 3 were a few times underestimated. We correct Table 5 and re-plot Figure 3 together with the unaffected curves. The program to calculate the corrected curves of growth is available at http://www.hp.phys.titech.ac.jp/kotani/cog/index.html
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Accretion disc winds in X-ray binaries
Accretion disc winds are a common, perhaps ubiquitous, feature of X-ray binaries, observed across multiple wavelengths and linked to disc atmospheres, jets and varying accretion states.