HSC 2874

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0.17 UTI
0.29
CN
0.25
Cdens
0.5
CC3
0.0
Clit
0.83
Cdup
Radius (P>50% members) 6.5 [arcmin]
  • CN 0.29 Poorly populated
  • Cdens 0.25 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.83 Very likely unique

Overview

â„šī¸
HSC 2874 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.

Note: This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry. See table with shared members information.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=0.83) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Relatively close High extinction Massive Near-solar metallicity Very young

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 259.085 -39.339 0.392 -0.472 -1.423 -43.017
Hunt & Reffert 2024 259.106 -39.314 0.394 -0.469 -1.45 40.246
Cavallo et al. 2024 259.087 -39.305 0.393 – – –
Hunt & Reffert 2023 259.106 -39.314 0.394 -0.469 -1.45 40.246

💡 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 – – – – – 1257* – –
Cavallo et al. 2024 2.75 4.23 – 11 0.300 – – –
Hunt & Reffert 2023 2.41 4.43 2.04 11 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 559 17.2 259.15 -39.65 0.39 -0.47 -1.42 -26.57 0.55

💡 Note: The % column shows the percentage of members that HSC 2874 shares with each listed object.

Visualization

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