HSC 249

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0.34 UTI
0.44
CN
1.0
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 16.0 [N/pc2]
  • CN 0.44 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 249 is a poorly populated, very dense object of low 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, 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.

Palma et al. (2025)
Part of multiple system G156, along with UBC_1033, HSC_250 and HSC_245.

Cavallo et al. (2024)
Bronze 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– 279.69 -6.567 0.42 0.337 -1.512 89.933
Hunt & Reffert 2024 279.694 -6.568 0.435 0.341 -1.526 89.942
Cavallo et al. 2024 279.691 -6.566 0.439 – – –
Hunt & Reffert 2023 279.694 -6.568 0.435 0.341 -1.526 89.942

💡 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– 2.435 4.2 1.91 84 0.280 662 – –
Hunt & Reffert 2024 – – – – – 662(1) – –
Cavallo et al. 2024 2.69 3.78 – 132 0.280 – – –
Hunt & Reffert 2023 2.18 4.62 1.91 36 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3785 100.0 279.69 -6.57 0.42 0.34 -1.51 4.9 0.07

💡 Note: The % column shows the percentage of members that HSC 249 shares with each listed object.

Visualization

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