HSC 2785

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0.48 UTI
0.8
CN
1.0
Cdens
0.62
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 46.9 [N/pc2]
  • CN 0.8 Rich
  • 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 2785 is a rich, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a very small percentage of members with at least one entry reported in the same catalogue. See table with shared members information.

Palma et al. (2025)
Part of multiple system G165, along with HSC_2778, NGC_6134, NGC_6193, Theia_1643, NGC_6204 and CWNU_1842.

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– 249.565 -48.797 0.831 1.245 -4.274 -19.258
Hunt & Reffert 2024 249.552 -48.802 0.815 1.243 -4.276 -32.776
Cavallo et al. 2024 249.549 -48.785 0.838 – – –
Hunt & Reffert 2023 249.552 -48.802 0.815 1.243 -4.276 -32.776

💡 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– 1.22 2.24 2.4 5 -0.220 747 – –
Hunt & Reffert 2024 – – – – – 747(1) – –
Cavallo et al. 2024 1.31 2.36 – 6 -0.220 – – –
Hunt & Reffert 2023 1.13 2.12 2.40 4 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Theia 1643 2.3 250.31 -48.97 0.84 0.8 -4.53 -28.04 0.2

💡 Note: The % column shows the percentage of members that HSC 2785 shares with each listed object.

Visualization

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