Table 1.
Pulsation and chemical properties for high-velocity RR Lyrae candidates found in our analysis.
| ID | P | AmpVCSS | Type | [Fe/H] |
|---|---|---|---|---|
| [day] | [mag] | [dex] | ||
| HV-RRL-01 | 0.33118 | 0.34221 | RRc | −0.90 ± 0.08 |
| HV-RRL-02 | 0.56564 | 0.91313 | RRab | −0.80 ± 0.13 |
| HV-RRL-03 (*) | 0.61772 | 0.17046 | RRab | −1.36 ± 0.19 |
| HV-RRL-04 (*) | 0.39219 | 0.26468 | RRc | −1.92 ± 0.19 |
| HV-RRL-05 | 0.36655 | 0.44251 | RRc | −1.78 ± 0.19 |
| HV-RRL-06 | 0.40890 | 0.74320 | RRab | −1.82 ± 0.19 |
| HV-RRL-07 | 0.75194 | 0.45923 | RRab | −1.64 ± 0.19 |
| HV-RRL-08 | 0.50023 | 0.97984 | RRab | −1.06 ± 0.19 |
| HV-RRL-09 | 0.35240 | 0.42820 | RRc | −1.55 ± 0.51 |
Notes.
The first column lists our adopted object ID. Columns (2) and (3) provide the star’s pulsation period, P, and amplitude of the total light changes based on the CSS photometry. In the last two columns, we list the assumed RR Lyrae sub-class and metallicity derived using the ΔS method. Similarly to Table B.1 we marked variables with an uncertain classification with an asterisk.
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.