NGC 2368
(Collinder 138; MWSC 1186; OCL 571)
0.20
UTI
0.0
CN
0.01
Cdens
0.12
CC3
0.44
Clit
1.0
Cdup
Nm (P>50%)
17
Core radius and density
10 [pc], 0.04 [pc-2]
- CN 0.0 Sparse
- Cdens 0.01 Very loose
- CC3 0.12 Very low quality
- Clit 0.44 Poorly studied
- Cdup 1.0 Unique
Overview
NGC 2368 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a massive, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999β | 110.264 | -10.339 | 0.256 | -1.435 | 1.285 | 68.186 |
| Just et al. | 2023 | 110.266 | -10.333 | β | β | β | β |
| Bica et al. | 2019 | 110.271 | -10.366 | β | β | β | β |
| Kharchenko et al. | 2016 | 110.266 | -10.333 | β | β | β | β |
| Kharchenko et al. | 2013 | 110.272 | -10.335 | β | 0.6 | 4.36 | β |
| Dias et al. | 2002 | 110.275 | -10.372 | β | β | β | β |
| Lynga | 1987 | 110.236 | -10.385 | β | β | β | β |
| Sulentic et al. | 1973 | 110.247 | -10.381 | β | β | β | β |
| Alter et al. | 1970 | 110.236 | -10.385 | 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 | 4.89 | 1.51 | β | 944 | β | 1774 | β | β |
| Just et al. | 2023 | β | β | β | 944 | β | 1774 | β | β |
| Kharchenko et al. | 2016 | 4.89 | 1.51 | β | 944 | β | β | β | β |
| Kharchenko et al. | 2013 | 4.89 | 1.51 | β | 944 | β | β | β | β |
| Dias et al. | 2002 | β | 0.38 | β | 50 | β | β | β | β |
MOCA

Dias et al. (2016)
No cluster (Piatti, A. E.; ClariΓ‘, J. J.; Ahumada, A. V. 2011, NewA 16, 161); cat V3.5 (Jan 2016)
Piatti et al. (2011)
Not a genuine open cluster.