NGC 2483
(MWSC 1383; OCL 677.1; ESO 430 02)
0.45
UTI
0.0
CN
0.09
Cdens
0.5
CC3
0.82
Clit
1.0
Cdup
Radius (P>50% members)
5.6 [arcmin]
- CN 0.0 Sparse
- Cdens 0.09 Very loose
- CC3 0.5 Intermediate quality
- Clit 0.82 Well-studied
- Cdup 1.0 Unique
Overview
NGC 2483 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is well-studied in the literature.
(*): The parallax distance estimate (~4.08 kpc) differs significantly from the median photometric distance (~1.66 kpc).
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
Relatively close
Low extinction
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 118.888 | -28.001 | 0.245 | -2.3 | 3.272 | â |
| Hunt & Reffert | 2024 | 118.879 | -27.945 | 0.237 | -2.285 | 3.255 | â |
| Cavallo et al. | 2024 | 118.907 | -28.042 | 0.238 | â | â | â |
| Hunt & Reffert | 2023 | 118.879 | -27.945 | 0.237 | -2.285 | 3.255 | â |
| Just et al. | 2023 | 118.915 | -27.902 | â | â | â | â |
| Bica et al. | 2019 | 118.928 | -27.897 | â | â | â | â |
| Loktin & Popova | 2017 | 118.92 | -27.894 | â | -2.714 | 0.133 | 121.51 |
| Kharchenko et al. | 2016 | 118.915 | -27.902 | â | â | â | â |
| Dias et al. | 2014 | 118.912 | -27.895 | â | -2.01 | 0.55 | 121.51 |
| Kharchenko et al. | 2013 | 118.92 | -27.905 | â | -1.0 | 2.45 | â |
| Piskunov et al. | 2008 | 118.903 | -27.899 | â | â | â | â |
| van den Bergh | 2006 | 118.9 | -27.9 | â | â | â | â |
| Kharchenko et al. | 2005 | 118.9 | -27.9 | â | -2.24 | 1.55 | â |
| Kharchenko et al. | 2003 | 118.96 | -27.91 | â | -2.18 | 1.64 | â |
| Dias et al. | 2002 | 118.912 | -27.895 | â | -2.01 | 0.55 | 121.51 |
| Dambis | 1999 | 118.9 | -27.9 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Hunt & Reffert | 2024 | â | â | â | â | â | 142* | â | â |
| Cavallo et al. | 2024 | 3.37 | 0.64 | â | 186 | 0.230 | â | â | â |
| Hunt & Reffert | 2023 | 3.82 | 0.70 | 1.71 | 107 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 40 | â | 123 | â | â |
| Loktin & Popova | 2017 | 1.73 | 0.87 | â | 19 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.65 | 1.10 | â | 40 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.65 | 1.10 | â | 40 | â | â | â | â |
| Piskunov et al. | 2008 | 1.66 | 0.93 | â | 31 | â | â | â | â |
| van den Bergh | 2006 | 1.66 | 0.93 | â | 12 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.66 | 0.93 | â | 31 | â | â | â | â |
| Kharchenko et al. | 2003 | 1.67 | 0.93 | â | â | â | â | â | â |
| Dias et al. | 2002 | 1.66 | 0.94 | â | 12 | â | â | â | â |
| Dambis | 1999 | 2.01 | 1.40 | â | 3 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.