HSC 1853

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0.38 UTI
0.26
CN
1.0
Cdens
0.62
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 9.5 [N/pc2]
  • CN 0.26 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1853 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age 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.

Palma et al. (2025)
Classified as genetic pair P210, along with DBSB_9.

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 99999– 112.749 -18.93 0.264 -1.992 2.354 –
Hunt & Reffert 2024 112.746 -18.935 0.263 -2.007 2.366 –
Cavallo et al. 2024 112.74 -18.928 0.263 – – –
Hunt & Reffert 2023 112.746 -18.935 0.263 -2.007 2.366 –

💡 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– 3.39 2.255 1.65 90 0.450 360 – –
Hunt & Reffert 2024 – – – – – 360(1) – –
Cavallo et al. 2024 2.99 1.98 – 162 0.450 – – –
Hunt & Reffert 2023 3.79 2.53 1.65 19 – – – –

(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 4132 88.5 112.75 -18.93 0.27 -1.99 2.36 – 0.02

💡 Note: The % column shows the percentage of members that HSC 1853 shares with each listed object.

Visualization

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