HSC 1289

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0.30 UTI
0.31
CN
0.17
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 7.2 [arcmin]
  • CN 0.31 Poorly populated
  • Cdens 0.17 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 1289 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 84.727 46.11 0.348 -0.24 -1.553 29.865
Zhang et al. 2024 84.712 46.158 – – – –
Hunt & Reffert 2024 84.712 46.158 0.337 -0.214 -1.508 79.971
Cavallo et al. 2024 84.703 46.113 0.336 – – –
Hunt & Reffert 2023 84.712 46.158 0.337 -0.214 -1.508 79.971

💡 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
Zhang et al. 2024 – – – – -0.299* – – –
Hunt & Reffert 2024 – – – – – 165* – –
Cavallo et al. 2024 2.51 1.44 – 83 -0.140 – – –
Hunt & Reffert 2023 2.58 1.05 0.66 151 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3540 74.2 84.74 46.07 0.34 -0.26 -1.55 50.11 0.02

💡 Note: The % column shows the percentage of members that HSC 1289 shares with each listed object.

Visualization

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