Mon OB1-D
0.39
UTI
0.9
CN
1.0
Cdens
0.75
CC3
0.35
Clit
0.58
Cdup
Stellar density (N50/rad)
110.2 [N/pc2]
- CN 0.9 Very rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.35 Poorly studied
- Cdup 0.58 Likely unique
Overview
Mon OB1-D is a very rich, very dense object of high 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, very young cluster, but with a large variance across recent sources for the absorption and mass parameters (see Parameters). It was recently reported in the literature.
Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. 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 | 99999â | 100.246 | 9.621 | 1.378 | -2.089 | -3.702 | 21.972 |
| Wei et al. | 2025 | 100.226 | 9.724 | 1.396 | -1.862 | -3.671 | â |
| Zhang et al. | 2024 | 100.274 | 9.573 | â | â | â | â |
| Hunt & Reffert | 2024 | 100.274 | 9.573 | 1.378 | -2.378 | -3.723 | 21.55 |
| Cavallo et al. | 2024 | 100.277 | 9.595 | 1.376 | â | â | â |
| Hunt & Reffert | 2023 | 100.274 | 9.573 | 1.378 | -2.378 | -3.723 | 21.55 |
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 | 0.695 | 0.41 | 1.61 | 10 | 0.250 | 760 | 0.58 | â |
| Liu et al. | 2025 | 0.70 | 0.07 | â | 8 | â | â | â | â |
| Wei et al. | 2025 | 0.61 | 0.38 | â | 13 | 0.250 | 1408 | 0.58 | â |
| Zhang et al. | 2024 | â | â | â | â | 0.203(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 112(1) | â | â |
| Cavallo et al. | 2024 | 0.88 | 0.74 | â | 28 | 0.330 | â | â | â |
| Hunt & Reffert | 2023 | 0.69 | 0.44 | 1.61 | 6 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Liu et al. (2025)
Classified as primordial binary cluster 274 along with NGC_2264.
Palma et al. (2025)
Classified as optical pair (not dynamically associated) P235, along with NGC_2264.
Cavallo et al. (2024)
Wood sample.