HSC 2506

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0.25 UTI
0.49
CN
0.37
Cdens
0.5
CC3
0.0
Clit
0.92
Cdup
Radius (P>50% members) 4.2 [arcmin]
  • CN 0.49 Poorly populated
  • Cdens 0.37 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.92 Very likely unique

Overview

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HSC 2506 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

Note: This is very likely a unique object, which shares a very small percentage of members with at least one previously reported entry. See table with shared members information.

Distant High extinction Massive Near-solar metallicity Young

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 185.53 -62.307 0.236 -6.487 0.418 31.112
Hunt & Reffert 2024 185.501 -62.3 0.228 -6.479 0.411 –
Cavallo et al. 2024 185.537 -62.311 0.228 – – –
Hunt & Reffert 2023 185.501 -62.3 0.228 -6.479 0.411 –

💡 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 – – – – – 2530* – –
Cavallo et al. 2024 3.58 4.32 – 23 -0.040 – – –
Hunt & Reffert 2023 3.99 3.14 2.75 96 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3787 51.0 185.53 -62.31 0.24 -6.49 0.41 72.51 0.0
FoF 1595 8.2 185.66 -62.43 0.25 -6.62 0.38 -25.58 0.03

💡 Note: The % column shows the percentage of members that HSC 2506 shares with each listed object.

Visualization

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