HSC 2006

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0.08 UTI
0.46
CN
0.5
Cdens
0.75
CC3
0.0
Clit
0.24
Cdup
Radius (P>50% members) 3.7 [arcmin]
  • CN 0.46 Poorly populated
  • Cdens 0.5 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.24 Likely duplicate

Overview

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HSC 2006 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a moderate 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.

âš ī¸ Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Distant 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 – 121.458 -31.601 0.251 -2.456 2.828 –
Hunt & Reffert 2024 121.454 -31.594 0.251 -2.455 2.825 –
Cavallo et al. 2024 121.442 -31.583 0.251 – – –
Hunt & Reffert 2023 121.454 -31.594 0.251 -2.455 2.825 –

💡 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 – – – – – 296* – –
Cavallo et al. 2024 3.30 1.42 – 83 -0.040 – – –
Hunt & Reffert 2023 3.44 0.98 0.84 124 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 204 76.1 121.44 -31.6 0.24 -2.45 2.85 – 0.27
Ruprecht 155 10.9 121.27 -31.81 0.25 -2.44 2.81 – 0.26

💡 Note: The % column shows the percentage of members that HSC 2006 shares with each listed object.

Visualization

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