Table 3
Best fits of the EPIC spectra of the two Oe stars with thermal plasma models.
| Star | d.o.f. |
|
N H | log Nwind | k T 1 | k T 2 | norm2/norm1 |
|
|
| (1022 cm-2) | (cm-2) | (keV) | (keV) | (erg cm-2 s-1) | (erg cm-2 s-1) | ||||
|
|
|||||||||
| HD 45314 | 225 | 1.16 | 0.19 (fixed) |
|
|
– | – |
|
|
| HD 60848 | 16 | 1.21 | 0.03 (fixed) | – |
|
|
0.13 ± 0.11 |
|
|
Notes.The last two columns yield the observed and absorption-corrected fluxes over the 0.5–10.0 keV energy range. The errors were estimated using the cflux and flux err commands in xspec. The relative errors on the fluxes are very similar to those on the source count rates.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.