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 |
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| * |
The launch of
ASCA enabled the
|
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|
first X-ray
spectra of cosmic
|
|
|
sources with CCD
resolution -
|
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|
roughly 5 - 6
times better than the
|
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|
resolution
achievable with the
|
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|
earlier prop
counter experiments.
|
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| * |
Observations of
stellar coronae
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|
indicated the
presence of multiple
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temperature
components, as well as
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|
anomalous
abundances for O, Ne,
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|
Mg, Si, S, and
Fe.
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| * |
This spectrum of
RZ Cas (an Algol
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|
binary) indicated
subsolar
|
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|
abundances by
factors of 2 - 5, very
|
|
similar to what
had been found for
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|
RS CVn’s, but not
for less active
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single stars.
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Singh,
Drake, and White, 1995,
|
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Ap.J.,445,
840.
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