Graham 1

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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

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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

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

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 164.134 -63.008 0.265 -6.261 2.178 47.507
Almeida et al. 2025 164.148 -63.017 – – – –
Celli et al. 2024 164.134 -63.018 – – – –
Dias et al. 2021 164.148 -63.017 0.222 -6.338 2.148 –
Cantat-Gaudin et al. 2020 164.134 -63.018 0.218 -6.324 2.178 –
SΓ‘nchez et al. 2020 164.133 -63.018 – -6.536 2.048 –
Cantat-Gaudin & Anders 2020 164.134 -63.018 0.218 -6.324 2.178 –
Monteiro & Dias 2019 164.134 -63.018 – -6.303 2.164 2.598
Soubiran et al. 2018 164.134 -63.018 – – – 3.88
Cantat-Gaudin et al. 2018 164.134 -63.018 0.218 -6.324 2.178 –
Dias et al. 2014 164.133 -63.018 – -3.17 1.91 –
Dias et al. 2002 164.133 -63.018 – -6.99 4.89 –

πŸ’‘ 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 – 6 – 153 – –
Celli et al. 2024 – – – 16 – 262 – –
Dias et al. 2021 3.65 2.21 – 6 -0.003 – – –
Cantat-Gaudin et al. 2020 3.56 2.29 – 15 – – – –
Cantat-Gaudin & Anders 2020 4.06 – – – – – – –
Monteiro & Dias 2019 4.94 2.12 – 8 0.039 – – –
Soubiran et al. 2018 4.06 – – – – – – –
Cantat-Gaudin et al. 2018 4.06 – – – – – – –
Dias et al. 2002 3.60 – – – – – – –

Visualization

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