HSC 2141

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0.38 UTI
0.5
CN
1.0
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 2.0 [arcmin]
  • CN 0.5 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2141 is a moderately populated, very dense object of low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high 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 large percentage of members with a later reported entry. See table with shared members information.

Distant High extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Bronze sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 132.861 -45.851 0.215 -3.784 4.065 51.214
Hunt & Reffert 2024 132.876 -45.85 0.217 -3.737 4.087 51.131
Cavallo et al. 2024 132.864 -45.844 0.212 – – –
Hunt & Reffert 2023 132.876 -45.85 0.217 -3.737 4.087 51.131

💡 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 – – – – – 928* – –
Cavallo et al. 2024 4.45 3.91 – 102 -0.040 – – –
Hunt & Reffert 2023 4.15 4.02 2.11 128 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3045 100.0 132.87 -45.85 0.22 -3.79 4.03 44.09 0.24

💡 Note: The % column shows the percentage of members that HSC 2141 shares with each listed object.

Visualization

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