Free Access
Table 5
Other X-ray sources in the field with 2MASS counterpart non-members of η Chamaleontis.
2MASS | J | H | KS | Note |
(mag) | (mag) | (mag) | ||
|
||||
J08394669-7900026 | 17.21 ± 0.22 | 16.42 ± 0.22 | 15.56 ± 0.23 | Galaxy |
J08431595-7853422 | 14.95 ± 0.03 | 14.25 ± 0.04 | 14.00 ± 0.06 | M-type |
J08440921-7906156 | 15.31 ± 0.05 | 14.53 ± 0.06 | 14.41 ± 0.07 | K-M giant |
J08451844-7854426 | 13.16 ± 0.03 | 12.69 ± 0.02 | 12.63 ± 0.03 | K-type |
J08483486-7853513 | 12.22 ± 0.02 | 11.69 ± 0.03 | 11.40 ± 0.02 | dM5e* |
Notes.
(*)
Lawson et al. (2002) rejected this star as a cluster member and gave spectral type M5 with emission. Luhman (2004) later confirmed this result.
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.