Harvard 9
(MWSC 2304; OCL 944; ESO 177 08)
0.18
UTI
0.0
CN
0.03
Cdens
0.12
CC3
0.38
Clit
1.0
Cdup
Radius (P>50% members)
8.0 [arcmin]
- CN 0.0 Sparse
- Cdens 0.03 Very loose
- CC3 0.12 Very low quality
- Clit 0.38 Poorly studied
- Cdup 1.0 Unique
Overview
Harvard 9 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 an intermediate-age cluster (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~4.14 kpc) differs significantly from the median photometric distance (~1.48 kpc).
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Relatively close
Moderate extinction
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 233.464 | -53.697 | 0.241 | -7.369 | -5.145 | -118.062 |
| Just et al. | 2023 | 233.448 | -53.679 | â | â | â | â |
| Bica et al. | 2019 | 233.443 | -53.677 | â | â | â | â |
| Kharchenko et al. | 2016 | 233.448 | -53.679 | â | â | â | â |
| Dias et al. | 2014 | 233.442 | -53.667 | â | -1.81 | -2.53 | â |
| Kharchenko et al. | 2013 | 233.46 | -53.68 | â | -4.21 | -2.97 | â |
| Dias et al. | 2002 | 233.442 | -53.667 | â | -1.81 | -2.53 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Just et al. | 2023 | â | â | â | 178 | â | 142 | â | â |
| Kharchenko et al. | 2016 | 1.48 | 2.90 | â | 178 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.48 | 2.90 | â | 178 | â | â | â | â |
| Dias et al. | 2002 | 1.48 | 2.90 | â | 178 | â | â | â | â |
