HSC 2785

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0.48 UTI
0.8
CN
1.0
Cdens
0.62
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 6.2 [arcmin]
  • 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.

Relatively close Moderate extinction Near-solar metallicity Very young

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 – 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] Bfr BSS
Hunt & Reffert 2024 – – – – – 747* – –
Cavallo et al. 2024 1.31 2.36 – 6 -0.220 – – –
Hunt & Reffert 2023 1.13 2.12 2.40 4 – – – –

(*): Indicates that this parameter is assigned more than one value 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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