HSC 2800

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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) 2.2 [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 2800 is a sparse, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a very metal-poor, young cluster (see Parameters). It was recently reported in the literature.

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

Distant High extinction Very metal-poor 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 – 249.181 -46.324 0.327 -2.245 -3.881 -48.265
Hunt & Reffert 2024 249.188 -46.323 0.319 -2.246 -3.874 -24.448
Cavallo et al. 2024 249.165 -46.315 0.319 – – –
Hunt & Reffert 2023 249.188 -46.323 0.319 -2.246 -3.874 -24.448

💡 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 – – – – – 741* – –
Cavallo et al. 2024 3.09 4.46 – 60 -1.150 – – –
Hunt & Reffert 2023 3.10 3.85 2.09 102 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3774 76.0 249.19 -46.32 0.33 -2.24 -3.89 -38.15 0.07

💡 Note: The % column shows the percentage of members that HSC 2800 shares with each listed object.

Visualization

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