HSC 2830

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0.51 UTI
0.28
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.3 [arcmin]
  • CN 0.28 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 2830 is a poorly 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 near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (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.

Relatively close High 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 – 253.302 -45.029 0.364 -0.474 -2.577 -8.314
Hu & Soubiran 2025 253.315 -45.031 – – – –
Hunt & Reffert 2024 253.292 -45.036 0.369 -0.502 -2.584 -9.837
Cavallo et al. 2024 253.315 -45.031 0.369 – – –
Hunt & Reffert 2023 253.292 -45.036 0.369 -0.502 -2.584 -9.837

💡 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
Hu & Soubiran 2025 – – – – -0.400* – – –
Hunt & Reffert 2024 – – – – – 531* – –
Cavallo et al. 2024 2.23 3.78 – 562 0.000 – – –
Hunt & Reffert 2023 2.44 3.56 2.42 33 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3746 96.4 253.31 -45.03 0.36 -0.47 -2.58 -8.31 0.04

💡 Note: The % column shows the percentage of members that HSC 2830 shares with each listed object.

Visualization

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