Table 2
Radio HII regions in the direction of HESS J1912+101.
| Label | Name | WISE | v (km s−1) | D (kpc) | Ref. |
|---|---|---|---|---|---|
| A | U44.26+0.10 | G044.257+00.095 | 59.6 | 7.8 | 1,2 |
| B | G044.427−0.317 | G044.427−00.317 | 61.1 | 7.7 | 3,4 |
| C | G044.501+0.335 | G044.501+00.332 | −43.0 | 15.5 | 3,4 |
| G044.518+0.379 | G044.521+00.385 | −49.7 | 16.2 | 3,4 | |
| D | G044.528−0.234 | G044.552−00.239 | 58.4 | 7.9 | 3,4 |
| E | D44.79−0.49 | G044.811−00.492 | 44.8 | 8.9 | 1,2 |
Notes. The “Label’ column refers to Fig. 1. For sources A and E, the “Name” of the radio HII regions is taken from reference (2), while for sources B, C, and D it is taken from reference (3). The “WISE” column shows the associated infrared source from the WISE Catalog of Galactic HII Regions (Anderson et al. 2014). The column “υ” reports the systemic velocity reported in the references, and “D” is the corresponding kinematic distance using the Reid14 Galactic rotation model.
References. (1) Lockman (1989), (2) Anderson et al. (2009), (3) Anderson et al. (2011), and (4) Anderson et al. (2012).
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.