Open Access
Table 2
X-ray-undetected Wolf–Rayet stars in Wd1.
| Name | Other | RA | Dec | Spectral type |
|---|---|---|---|---|
| names | h m s | ° ′ ″ | ||
| (1) | (2) | (3) | (4) | (5) |
| C | WR77m | 16:47:04.40 | −45:51:03.8 | WC9d |
| K | WR77g | 16:47:03.25 | −45:50:43.8 | WC8 |
| M | WR77i, W66 | 16:47:03.96 | −45:51:37.5 | WC9d |
| T | WR77aa | 16:46:46.3 | −45:47:58.0 | WC9d(a) |
Notes. Same as in Table 1 apart from coordinate values that are obtained from Clark et al. (2020). The luminosity upper limit in the 0.5–8.0 keV band for the undetected sources is 1.4 × 1029 erg s−1 (we describe in detail its derivation in Sec. 4.2).(a)Hopewell et al. (2005).
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.