| X-Ray Binary Sources:� Then
Again |
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| * | The ASCA Solid
State Imaging |
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| Spectrometer
observation of Cyg X- |
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| 3 did indeed
confirm the presence of |
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| Fe K emission in
the spectrum, but |
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| indicated that it
was far from the |
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| most prominent
feature. |
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| * | Liedahl &
Paerels showed that in |
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| addition to
H-like and He-like line |
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| emission from
lower-Z elements, we |
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| also see narrow
radiative |
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| recombination
continua (RRCs). |
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| * | These indicate
that the line emitting |
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| gas is
photoionized - suspected, but |
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| never previously
demonstrated for |
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| accretion-powered
sources. |
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| Liedahl
& Paerels, 1996, Ap. J., 468, L33. |