HSC 2561

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0.02 UTI
0.66
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.04
Cdup
Stellar density (N50/rad) 24.9 [N/pc2]
  • CN 0.66 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.04 Very likely duplicate

Overview

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HSC 2561 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, metal-poor, intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It was recently reported in the literature.

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

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 99999– 197.62 -63.398 0.239 -6.416 -1.232 -54.394
Hunt & Reffert 2024 197.613 -63.397 0.236 -6.415 -1.219 -50.757
Cavallo et al. 2024 197.627 -63.401 0.229 – – –
Hunt & Reffert 2023 197.613 -63.397 0.236 -6.415 -1.219 -50.757

💡 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] Bfrac BSS
UCC 99999– 3.36 4.135 2.4 284 -0.690 1949 – –
Hunt & Reffert 2024 – – – – – 1949(1) – –
Cavallo et al. 2024 2.75 4.01 – 490 -0.690 – – –
Hunt & Reffert 2023 3.97 4.26 2.40 78 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 1142 96.4 197.62 -63.4 0.24 -6.41 -1.21 -54.21 0.5

💡 Note: The % column shows the percentage of members that HSC 2561 shares with each listed object.

Visualization

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