HSC 2580

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0.40 UTI
0.0
CN
1.0
Cdens
1.0
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 1.1 [arcmin]
  • CN 0.0 Sparse
  • 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 2580 is a sparse, very dense object of very high C3 quality. Its parallax locates it at a large* distance, below the mid-plane, affected by high extinction. It is catalogued as a metal-poor, young cluster (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~5.37 kpc) differs significantly from the median photometric distance (~3.54 kpc).

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Distant High extinction Metal-poor Young

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 – 200.33 -63.431 0.186 -5.853 -1.114 –
Hunt & Reffert 2024 200.328 -63.433 0.185 -5.878 -1.109 –
Cavallo et al. 2024 200.314 -63.43 0.185 – – –
Hunt & Reffert 2023 200.328 -63.433 0.185 -5.878 -1.109 –

💡 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 – – – – – 689* – –
Cavallo et al. 2024 2.17 3.04 – 85 -0.650 – – –
Hunt & Reffert 2023 4.90 3.20 1.98 15 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3354 88.0 200.33 -63.43 0.19 -5.85 -1.12 – 0.05

💡 Note: The % column shows the percentage of members that HSC 2580 shares with each listed object.

Visualization

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