HSC 1538

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0.32 UTI
0.34
CN
1.0
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 3.9 [arcmin]
  • CN 0.34 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1538 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a relatively close distance, near 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 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 – 93.02 16.224 0.513 -0.011 -3.045 -5.532
Hunt & Reffert 2024 93.018 16.224 0.513 0.013 -3.039 -2.509
Cavallo et al. 2024 93.013 16.222 0.515 – – –
Hunt & Reffert 2023 93.018 16.224 0.513 0.013 -3.039 -2.509

💡 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 – – – – – 247* – –
Cavallo et al. 2024 1.57 2.46 – 447 -0.260 – – –
Hunt & Reffert 2023 1.82 2.44 1.84 143 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3340 100.0 93.02 16.22 0.51 -0.01 -3.04 -5.45 0.09

💡 Note: The % column shows the percentage of members that HSC 1538 shares with each listed object.

Visualization

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