HSC 391

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0.29 UTI
0.26
CN
0.68
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 7.2 [arcmin]
  • CN 0.26 Poorly populated
  • Cdens 0.68 Moderately dense
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 391 is a poorly populated, moderately dense object of intermediate C3 quality. Its parallax locates it at a relatively close 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.

Relatively close 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 – 295.706 7.633 0.755 2.05 -0.796 -33.337
Hunt & Reffert 2024 295.729 7.611 0.744 1.971 -0.821 -30.552
Cavallo et al. 2024 295.717 7.657 0.744 – – –
Hunt & Reffert 2023 295.729 7.611 0.744 1.971 -0.821 -30.552

💡 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 – – – – – 94* – –
Cavallo et al. 2024 1.37 1.42 – 363 0.520 – – –
Hunt & Reffert 2023 1.26 1.55 1.98 238 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3196 92.3 295.71 7.63 0.76 2.06 -0.79 -33.34 0.02

💡 Note: The % column shows the percentage of members that HSC 391 shares with each listed object.

Visualization

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