HSC 2581

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0.48 UTI
0.41
CN
1.0
Cdens
1.0
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 0.9 [arcmin]
  • CN 0.41 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2581 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a large* 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.

(*): The parallax distance estimate (~5.07 kpc) differs significantly from the median photometric distance (~3.60 kpc).

Note: This object shares a large percentage of members with a later 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 – 200.999 -63.202 0.197 -5.894 -0.847 –
Hunt & Reffert 2024 201.007 -63.203 0.2 -5.924 -0.852 -42.21
Cavallo et al. 2024 201.019 -63.198 0.2 – – –
Hunt & Reffert 2023 201.007 -63.203 0.2 -5.924 -0.852 -42.21

💡 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 – – – – – 971* – –
Cavallo et al. 2024 2.55 2.24 – 380 -0.340 – – –
Hunt & Reffert 2023 4.65 2.26 2.37 34 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 2952 90.2 201.01 -63.2 0.2 -5.89 -0.86 -49.51 0.1

💡 Note: The % column shows the percentage of members that HSC 2581 shares with each listed object.

Visualization

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