HSC 1260

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0.40 UTI
0.27
CN
0.47
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 8.9 [arcmin]
  • CN 0.27 Poorly populated
  • Cdens 0.47 Loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 1260 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.

Note: This object shares a large 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 – 62.591 39.533 0.763 0.65 -2.861 -30.363
Zhang et al. 2024 62.562 39.541 – – – –
Hunt & Reffert 2024 62.562 39.541 0.751 0.623 -2.846 -28.121
Cavallo et al. 2024 62.529 39.488 0.748 – – –
Hunt & Reffert 2023 62.562 39.541 0.751 0.623 -2.846 -28.121

💡 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 – – – – 0.020* – – –
Hunt & Reffert 2024 – – – – – 118* – –
Cavallo et al. 2024 1.35 2.23 – 234 0.680 – – –
Hunt & Reffert 2023 1.26 2.43 0.94 185 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3019 100.0 62.61 39.53 0.76 0.64 -2.87 -30.36 0.05

💡 Note: The % column shows the percentage of members that HSC 1260 shares with each listed object.

Visualization

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