Lynga 6
(MWSC 2348)
0.98
UTI
0.88
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
5.3 [arcmin]
- CN 0.88 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Lynga 6 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a very metal-rich, young cluster, but with a large variance across recent sources for the age and mass parameters (see Parameters). It is very well-studied in the literature.
Relatively close
High extinction
Very metal-rich
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | β | 241.213 | -51.959 | 0.375 | -1.896 | -2.747 | -46.442 |
| Hunt & Reffert | 2024 | 241.221 | -51.965 | 0.376 | -1.909 | -2.747 | -33.494 |
| Celli et al. | 2024 | 241.218 | -51.96 | β | β | β | β |
| Cavallo et al. | 2024 | 241.197 | -51.965 | 0.377 | β | β | β |
| Hunt & Reffert | 2023 | 241.221 | -51.965 | 0.376 | -1.909 | -2.747 | -33.494 |
| Just et al. | 2023 | 241.212 | -51.924 | β | β | β | β |
| Jaehnig et al. | 2021 | 241.198 | -51.96 | 0.4 | -1.867 | -2.732 | β |
| Rain et al. | 2021 | 241.218 | -51.96 | 0.383 | -1.866 | -2.757 | β |
| Cantat-Gaudin et al. | 2020 | 241.218 | -51.96 | 0.383 | -1.866 | -2.757 | β |
| SΓ‘nchez et al. | 2020 | 241.217 | -51.933 | β | -1.836 | -2.78 | β |
| Cantat-Gaudin & Anders | 2020 | 241.218 | -51.96 | 0.383 | -1.866 | -2.757 | β |
| Soubiran et al. | 2018 | 241.218 | -51.96 | β | β | β | -46.6 |
| Cantat-Gaudin et al. | 2018 | 241.218 | -51.96 | 0.383 | -1.866 | -2.757 | β |
| Loktin & Popova | 2017 | 241.215 | -51.934 | β | -1.088 | -3.541 | -59.4 |
| Kharchenko et al. | 2016 | 241.212 | -51.924 | β | β | β | β |
| Dias et al. | 2014 | 241.217 | -51.933 | β | -2.61 | -4.01 | β |
| Kharchenko et al. | 2013 | 241.222 | -51.925 | β | -4.08 | -1.17 | -59.4 |
| Gozha et al. | 2012 | 241.217 | -51.933 | β | β | β | β |
| Kharchenko et al. | 2007 | 241.21 | -51.93 | β | 0.04 | β | β |
| van den Bergh | 2006 | 241.2 | -51.917 | β | β | β | β |
| Chen et al. | 2003 | 241.279 | -51.93 | β | -13.61 | -1.83 | -59.4 |
| Dias et al. | 2002 | 241.217 | -51.933 | β | -13.61 | -1.83 | -59.4 |
| Dambis | 1999 | 241.217 | -51.933 | β | β | β | β |
π‘ 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 |
|---|---|---|---|---|---|---|---|---|---|
| Hunt & Reffert | 2024 | β | β | β | β | β | 3856* | β | β |
| Celli et al. | 2024 | β | β | β | 3 | β | 454 | β | β |
| Cavallo et al. | 2024 | 2.86 | 3.86 | β | 26 | 1.060 | β | β | β |
| Hunt & Reffert | 2023 | 2.45 | 4.24 | 2.83 | 31 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 28 | β | 139 | β | β |
| Jaehnig et al. | 2021 | 2.52* | β | β | β | β | β | β | β |
| Rain et al. | 2021 | 2.43 | 3.88 | β | 27 | β | β | β | 0 |
| Cantat-Gaudin et al. | 2020 | 2.42 | 3.51 | β | 3 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 2.43 | β | β | β | β | β | β | β |
| Soubiran et al. | 2018 | 2.43 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 2.43 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 1.60 | 3.82 | β | 31 | β | β | β | β |
| Kharchenko et al. | 2016 | 1.77 | 3.94 | β | 28 | β | β | β | β |
| Kharchenko et al. | 2013 | 1.77 | 3.94 | β | 28 | β | β | β | β |
| Gozha et al. | 2012 | 1.60 | β | β | 27 | β | β | β | β |
| van den Bergh | 2006 | 1.60 | 3.88 | β | 27 | β | β | β | β |
| Chen et al. | 2003 | 1.60 | β | β | 20 | β | β | β | β |
| Dias et al. | 2002 | 1.60 | 3.88 | β | 27 | β | β | β | β |
| Dambis | 1999 | 2.04 | 4.20 | β | 45 | β | β | β | β |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Silver sample.