Table 3
Computed Lyman continuum flux of the hot stars of the CMa OB1 association.
| Star | Sp. Type | log |
|---|---|---|
| (SIMBAD) | (s−1) | |
| HD 54662(2) | O6.5 V (a) | 48.88 |
| HD 53975 | O7.5V z(c) | 48.61 |
| HD 57682(3) | O9.2IV(b) | 47.97 |
| HD 54879 | O9.7V(c) | 47.88 |
| HD 53974 | B2I a/ab(d) | – |
| HD 53755 | B1II/III(d) | – |
| HD 53456 | B1Ib/II(d) | – |
| HD 53367(4) | B0IV/Ve(e) | – |
| HD 53623(5) | B0V(f) | – |
Notes. Runaways are indicated in italics. (1)Values from Martins et al. (2005), Table 4. (2)This runaway could be a spectroscopic binary, both with spectral types O6.5V, according to Mossoux et al. (2018). (3) This runaway is ~ 5° away from the nebula (see Fig. 1). (4)Ionizes the IC 2177 nebula. (5)Ionizes the Sh 2-297 nebula.
References. For spectral types: (a)Mossoux et al. (2018); (b)Sota et al. (2014); (c)Sota et al. (2011); (d)Houk & Swift (1999); (e)Tjin A Djie et al. (2001); (f)Houk & Smith-Moore (1988).
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.