Graham 1
0.61
UTI
0.0
CN
1.0
Cdens
0.75
CC3
0.65
Clit
1.0
Cdup
Radius (P>50% members)
1.3 [arcmin]
- CN 0.0 Sparse
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.65 Moderately studied
- Cdup 1.0 Unique
Overview
Graham 1 is a sparse, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is moderately studied in the literature.
Distant
Moderate extinction
Near-solar metallicity
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | β | 164.134 | -63.008 | 0.265 | -6.261 | 2.178 | 47.507 |
| Almeida et al. | 2025 | 164.148 | -63.017 | β | β | β | β |
| Celli et al. | 2024 | 164.134 | -63.018 | β | β | β | β |
| Dias et al. | 2021 | 164.148 | -63.017 | 0.222 | -6.338 | 2.148 | β |
| Cantat-Gaudin et al. | 2020 | 164.134 | -63.018 | 0.218 | -6.324 | 2.178 | β |
| SΓ‘nchez et al. | 2020 | 164.133 | -63.018 | β | -6.536 | 2.048 | β |
| Cantat-Gaudin & Anders | 2020 | 164.134 | -63.018 | 0.218 | -6.324 | 2.178 | β |
| Monteiro & Dias | 2019 | 164.134 | -63.018 | β | -6.303 | 2.164 | 2.598 |
| Soubiran et al. | 2018 | 164.134 | -63.018 | β | β | β | 3.88 |
| Cantat-Gaudin et al. | 2018 | 164.134 | -63.018 | 0.218 | -6.324 | 2.178 | β |
| Dias et al. | 2014 | 164.133 | -63.018 | β | -3.17 | 1.91 | β |
| Dias et al. | 2002 | 164.133 | -63.018 | β | -6.99 | 4.89 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Almeida et al. | 2025 | 3.65 | 2.21 | β | 6 | β | 153 | β | β |
| Celli et al. | 2024 | β | β | β | 16 | β | 262 | β | β |
| Dias et al. | 2021 | 3.65 | 2.21 | β | 6 | -0.003 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 3.56 | 2.29 | β | 15 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 4.06 | β | β | β | β | β | β | β |
| Monteiro & Dias | 2019 | 4.94 | 2.12 | β | 8 | 0.039 | β | β | β |
| Soubiran et al. | 2018 | 4.06 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 4.06 | β | β | β | β | β | β | β |
| Dias et al. | 2002 | 3.60 | β | β | β | β | β | β | β |


Almeida et al. (2025)
Mass determination: worst fit. Isochrone match: intermediate fit.