NGC 1931
0.76
UTI
0.68
CN
1.0
Cdens
0.75
CC3
0.7
Clit
1.0
Cdup
Radius (P>50% members)
1.5 [arcmin]
- CN 0.68 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.7 Moderately studied
- Cdup 1.0 Unique
Overview
NGC 1931 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is moderately studied in the literature.
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
Relatively close
Moderate extinction
Near-solar metallicity
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | β | 82.851 | 34.226 | 0.436 | 0.216 | -2.028 | -20.833 |
| Hunt & Reffert | 2024 | 82.852 | 34.224 | 0.424 | 0.237 | -2.036 | -20.834 |
| Cavallo et al. | 2024 | 82.843 | 34.224 | 0.425 | β | β | β |
| Hunt & Reffert | 2023 | 82.852 | 34.224 | 0.424 | 0.237 | -2.036 | -20.834 |
| Jaehnig et al. | 2021 | 82.804 | 34.238 | 0.455 | 0.302 | -1.935 | β |
| SΓ‘nchez et al. | 2020 | 82.854 | 34.245 | β | 0.384 | -1.813 | β |
| Loktin & Popova | 2017 | 82.86 | 34.245 | β | -0.011 | -1.655 | β |
| Dias et al. | 2014 | 82.854 | 34.245 | β | -0.29 | -3.48 | β |
| Gozha et al. | 2012 | 82.854 | 34.245 | β | β | β | β |
| Glushkova et al. | 2010 | 82.858 | 34.214 | β | β | β | β |
| van den Bergh | 2006 | 82.861 | 34.249 | β | β | β | β |
| Dias et al. | 2002 | 82.854 | 34.245 | β | -0.29 | -3.48 | β |
| Dambis | 1999 | 82.861 | 34.249 | 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 | 459* | β | β |
| Cavallo et al. | 2024 | 1.98 | 1.11 | β | 83 | 0.260 | β | β | β |
| Hunt & Reffert | 2023 | 2.12 | 1.92 | 2.45 | 12 | β | β | β | β |
| Jaehnig et al. | 2021 | 2.26* | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 3.07 | 2.29 | β | 10 | β | β | β | β |
| Gozha et al. | 2012 | 3.09 | β | β | 10 | -0.060 | β | β | β |
| Glushkova et al. | 2010 | 1.00 | 6.11 | β | 10 | β | β | β | β |
| van den Bergh | 2006 | 3.09 | 2.29 | β | 10 | β | β | β | β |
| Dias et al. | 2002 | 2.30 | 2.29 | β | 2 | β | β | β | β |
| Dambis | 1999 | 2.19 | 1.68 | β | 13 | β | β | β | β |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Bronze sample.