Stock 16
0.53
UTI
0.31
CN
0.1
Cdens
0.25
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
6.2 [arcmin]
- CN 0.31 Poorly populated
- Cdens 0.1 Very loose
- CC3 0.25 Low quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Stock 16 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by moderate extinction. It is catalogued as a very young cluster (see Parameters). It is very well-studied in the literature.
(*): The parallax distance estimate (~4.40 kpc) differs significantly from the median photometric distance (~1.81 kpc).
Relatively close
Moderate extinction
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 199.773 | -62.615 | 0.228 | -6.54 | -0.972 | -31.499 |
| Celli et al. | 2024 | 199.86 | -62.622 | â | â | â | â |
| Jaehnig et al. | 2021 | 199.682 | -62.583 | 0.501 | -4.178 | -1.796 | â |
| Rain et al. | 2021 | 199.86 | -62.622 | 0.222 | -6.574 | -0.991 | â |
| Cantat-Gaudin et al. | 2020 | 199.86 | -62.622 | 0.222 | -6.574 | -0.991 | â |
| Cantat-Gaudin & Anders | 2020 | 199.86 | -62.622 | 0.222 | -6.574 | -0.991 | â |
| Soubiran et al. | 2018 | 199.86 | -62.622 | â | â | â | -38.11 |
| Cantat-Gaudin et al. | 2018 | 199.86 | -62.622 | 0.222 | -6.574 | -0.991 | â |
| Loktin & Popova | 2017 | 199.875 | -62.633 | â | -8.407 | 2.036 | -41.8 |
| Dias et al. | 2014 | 199.871 | -62.633 | â | -8.97 | -3.36 | â |
| Gozha et al. | 2012 | 199.871 | -62.633 | â | â | â | â |
| Piskunov et al. | 2008 | 199.691 | -62.505 | â | â | â | â |
| Kharchenko et al. | 2007 | 199.87 | -62.63 | â | 0.22 | â | -41.8 |
| van den Bergh | 2006 | 199.7 | -62.517 | â | â | â | â |
| Kharchenko et al. | 2005 | 199.69 | -62.51 | â | -3.31 | -0.03 | -41.8 |
| Kharchenko et al. | 2003 | 199.69 | -62.51 | â | -3.58 | 0.15 | â |
| Dias et al. | 2002 | 199.871 | -62.633 | â | -8.97 | -3.36 | -41.8 |
| Dambis | 1999 | 199.871 | -62.633 | â | â | â | â |
đĄ Note: The UCC values are estimated from its identified members.
| Reference | Year | Dist [kpc] | Av [mag] | DAv [mag] | Age [Myr] | [Fe/H] [dex] | Mass [Msun] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Celli et al. | 2024 | â | â | â | 6 | â | 340 | â | â |
| Jaehnig et al. | 2021 | 1.99* | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 3.99 | 1.61 | â | 8 | â | â | â | 0 |
| Cantat-Gaudin & Anders | 2020 | 3.99 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 3.99 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 3.99 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 1.66 | 1.54 | â | 8 | â | â | â | â |
| Gozha et al. | 2012 | 1.81 | â | â | 8 | â | 1413 | â | â |
| Piskunov et al. | 2008 | 1.64 | 1.49 | â | 6 | â | â | â | â |
| van den Bergh | 2006 | 1.64 | 1.52 | â | 8 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.64 | 1.49 | â | 6 | â | â | â | â |
| Kharchenko et al. | 2003 | 1.64 | 1.24 | â | â | â | â | â | â |
| Dias et al. | 2002 | 1.81 | 1.61 | â | 8 | â | â | â | â |
| Dambis | 1999 | 1.85 | 1.45 | â | 3 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

