HSC 1217

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0.33 UTI
0.28
CN
0.86
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 2.1 [arcmin]
  • CN 0.28 Poorly populated
  • Cdens 0.86 Dense
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1217 is a poorly populated, dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, intermediate-age cluster (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.

Distant Moderate extinction Metal-rich 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 – 62.564 47.846 0.239 -0.379 -0.865 -72.036
Hunt & Reffert 2024 62.552 47.846 0.203 -0.355 -0.858 -72.034
Cavallo et al. 2024 62.558 47.853 0.208 – – –
Hunt & Reffert 2023 62.552 47.846 0.203 -0.355 -0.858 -72.034

💡 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
Hunt & Reffert 2024 – – – – – 235* – –
Cavallo et al. 2024 4.99 2.92 – 186 0.650 – – –
Hunt & Reffert 2023 4.01 2.83 1.24 182 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3414 100.0 62.56 47.85 0.24 -0.38 -0.89 -72.04 0.05

💡 Note: The % column shows the percentage of members that HSC 1217 shares with each listed object.

Visualization

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