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§ |
Chandra ACIS bright soft
phase data
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è |
out of time events analysed
to recover piled-up spectrum
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§ |
Chandra observations cover
turn-off time for soft component
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è |
less than 6 weeks
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§ |
Very detailed high resolution
Chandra LETGS spectrum
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è |
Study of individual lines:
Stongly broadned
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è |
A blend of many lines/cont.
detected in 28-38 Å range
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è |
Temperatures and densities
from H- and He-like triplets
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è |
Unexpected lack of Fe lines
detected
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§ |
Study of all Chandra
ACIS and LETGS spectra
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è |
Evolution of X-ray flux (similar decay rates as for Nova
Cyg 1975)
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