NGC 281-east
(NGC 281E)
0.11
UTI
0.46
CN
0.04
Cdens
0.12
CC3
0.0
Clit
0.91
Cdup
Nm (P>50%)
46
Core radius and density
2.4 [pc], 0.2 [pc-2]
- CN 0.46 Poorly populated
- Cdens 0.04 Very loose
- CC3 0.12 Very low quality
- Clit 0.0 Rarely studied
- Cdup 0.91 Very likely unique
Overview
NGC 281-east is a poorly populated, very loose object of very low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane. It is catalogued as a cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 23 years.
Note: This is very likely a unique object, which shares a very small percentage of members with at least one previously reported entry. See table with shared members information.
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=0.91) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 13.532 | 56.58 | 0.354 | -2.773 | -0.86 | â |
| Lada & Lada | 2003 | 13.561 | 56.556 | â | â | â | â |
| Bica et al. | 2003 | 13.559 | 56.56 | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 2.1 | â | â | â | â | 57 | â | â |
| Lada & Lada | 2003 | 2.10 | â | â | â | â | 57 | â | â |
MOCA

Bica et al. (2003)
Classified as infrared cluster (IRC).
Lada & Lada (2003)
Embedded cluster within âŧ2 Kpc of the Sun.