C-19_346.20-10.70

The Pristine survey - XVII. The C-19 stream is dynamically hot and more extended than previously thought
| Teff : 4966 | log g : 2.06 | vturb : 1.88 |
| Original Data | Converted Data Asplund et al. (2009) | |||||||
|---|---|---|---|---|---|---|---|---|
| Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
| C | N/A | -3.11+-0.3 | ... | ... | -3.04+-0.3 | 0.45+-0.3 | 5.39+-0.3 | C |
| Na | 1 | -3.10 | ... | ... | -4.04 | -0.55 | 2.20 | Na |
| Mg | 2 | -2.79+-0.01 | ... | ... | -2.85+-0.01 | 0.64+-0.01 | 4.75+-0.01 | Mg |
| Al | 2 | -3.87+-0.09 | ... | ... | -3.85+-0.09 | -0.36+-0.09 | 2.60+-0.09 | Al |
| Ca I | 3 | -2.99+-0.06 | ... | ... | -3.00+-0.06 | 0.49+-0.06 | 3.34+-0.06 | Ca I |
| Sc II | 1 | -3.02 | ... | ... | -3.07 | 0.42 | 0.08 | Sc II |
| Ti I | 2 | -2.95+-0.14 | ... | ... | -3.00+-0.14 | 0.49+-0.14 | 1.95+-0.14 | Ti I |
| Ti II | 7 | -2.87+-0.23 | ... | ... | -2.92+-0.23 | 0.57+-0.23 | 2.03+-0.23 | Ti II |
| Mn I | 1 | -4.34 | ... | ... | -4.40 | -0.91 | 1.03 | Mn I |
| Fe I | 33 | -3.51+-0.19 | ... | ... | -3.49+-0.19 | ... | 4.01+-0.19 | Fe I |
| Fe II | 1 | -3.41 | ... | ... | -3.39 | ... | 4.11 | Fe II |
| Co | 4 | -3.09+-0.20 | ... | ... | -3.16+-0.20 | 0.33+-0.20 | 1.83+-0.20 | Co |
| Ni | 3 | -3.32+-0.27 | ... | ... | -3.31+-0.27 | 0.18+-0.27 | 2.91+-0.27 | Ni |
| Sr | 2 | -3.80+-0.01 | ... | ... | -3.75+-0.01 | -0.26+-0.01 | -0.88+-0.01 | Sr |
| Binarity | Negative |
| Vrad | -133.5+-0.4 |
| Right Ascension : 23 04 48.77 | Declination : -10 41 47.40 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|---|---|---|---|---|---|
| 2021-05-18 | N/A | VLT | 40000 | N/A | 1800 | -133.5+-0.4 |
| 2021-10-23 | N/A | VLT | 40000 | N/A | N/A | -133.5+-0.4 |