NGC 1896
(MWSC 537)
0.28
UTI
0.31
CN
0.03
Cdens
0.38
CC3
0.35
Clit
1.0
Cdup
Nm (P>50%)
31
Core radius and density
5.1 [pc], 0.1 [pc-2]
- CN 0.31 Poorly populated
- Cdens 0.03 Very loose
- CC3 0.38 Low quality
- Clit 0.35 Poorly studied
- Cdup 1.0 Unique
Overview
NGC 1896 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age parameter (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 | 99999â | 81.319 | 29.273 | 1.18 | 3.189 | -6.007 | -7.826 |
| Hunt & Reffert | 2024 | 81.475 | 29.228 | 1.172 | 3.219 | -6.04 | -9.316 |
| Cavallo et al. | 2024 | 81.252 | 29.436 | 1.186 | â | â | â |
| Hunt & Reffert | 2023 | 81.475 | 29.228 | 1.172 | 3.219 | -6.04 | -9.316 |
| Just et al. | 2023 | 81.405 | 29.26 | â | â | â | â |
| Bica et al. | 2019 | 81.409 | 29.298 | â | â | â | â |
| Loktin & Popova | 2017 | 81.42 | 29.329 | â | 0.524 | -1.241 | â |
| Sampedro et al. | 2017 | 81.425 | 29.328 | â | 2.01 | -3.67 | â |
| Kharchenko et al. | 2016 | 81.405 | 29.26 | â | â | â | â |
| Dias et al. | 2014 | 81.425 | 29.328 | â | 1.89 | -4.35 | â |
| Kharchenko et al. | 2013 | 81.414 | 29.26 | â | 1.18 | -1.39 | â |
| Kharchenko et al. | 2012 | 81.414 | 29.26 | â | 1.18 | -1.39 | â |
| Piskunov et al. | 2008 | 81.409 | 29.298 | â | â | â | â |
| Kharchenko et al. | 2005 | 81.42 | 29.3 | â | 0.54 | -8.03 | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 0.86 | 0.85 | 0.51 | 945 | 0.360 | 154 | â | â |
| Hunt & Reffert | 2024 | 0.80 | 0.85 | 0.51 | 238 | â | 41(1) | â | â |
| Cavallo et al. | 2024 | 0.86 | 0.75 | â | 437 | 0.360 | â | â | â |
| Hunt & Reffert | 2023 | 0.80 | 0.85 | 0.51 | 238 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 1259 | â | 267 | â | â |
| Loktin & Popova | 2017 | 2.45 | 1.09 | â | 1549 | â | â | â | â |
| Kharchenko et al. | 2016 | 2.60 | 1.89 | â | 1259 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.60 | 1.89 | â | 1259 | â | â | â | â |
| Kharchenko et al. | 2012 | 2.60 | 1.89 | â | 1259 | â | â | â | â |
| Piskunov et al. | 2008 | 0.82 | 0.47 | â | 631 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.82 | 0.47 | â | 631 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 1.00 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (50th percentile).