NGC 2239
0.43
UTI
0.47
CN
0.52
Cdens
0.75
CC3
0.19
Clit
1.0
Cdup
Nm (P>50%)
47
Core radius and density
1.1 [pc], 2.6 [pc-2]
- CN 0.47 Poorly populated
- Cdens 0.52 Moderately dense
- CC3 0.75 High quality
- Clit 0.19 Rarely studied
- Cdup 1.0 Unique
Overview
NGC 2239 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a relatively close* distance, near the mid-plane, affected by high extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 6 years.
(*): The parallax distance estimate (~1.49 kpc) differs significantly from the median photometric distance (~3.51 kpc).
Note: This object shares a moderate percentage of members with at least one entry reported in the same catalogue. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999β | 97.756 | 4.939 | 0.673 | -1.834 | 0.029 | 24.063 |
| SΓ‘nchez et al. | 2020 | 97.737 | 4.969 | β | -1.614 | -0.338 | β |
| Dias et al. | 2018 | β | β | β | -3.0 | -1.16 | β |
| Loktin & Popova | 2017 | 97.74 | 4.97 | β | -0.6 | -2.18 | β |
| Sampedro et al. | 2017 | 97.737 | 4.969 | β | 0.01 | -0.78 | β |
| Dias et al. | 2014 | 97.737 | 4.969 | β | -0.6 | -2.18 | β |
| Dias et al. | 2002 | 97.737 | 4.969 | β | -0.6 | -2.18 | β |
| Lynga | 1987 | 97.727 | 4.953 | β | β | β | β |
| Sulentic et al. | 1973 | 97.733 | 4.948 | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999β | 3.51 | 3.02 | β | 304 | β | β | β | β |
| Loktin & Popova | 2017 | 3.12 | 2.57 | β | 603 | β | β | β | β |
| Dias et al. | 2002 | 3.90 | 3.47 | β | 5 | β | β | β | β |
MOCA
