HSC 2879

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0.11 UTI
0.0
CN
0.05
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 7.2 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.05 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 2879 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as an extremely massive, near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Distant High extinction Extremely massive Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Wood sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 257.117 -37.549 0.247 -1.196 -2.295 -51.368
Hunt & Reffert 2024 257.054 -37.547 0.262 -1.164 -2.309 -39.259
Cavallo et al. 2024 257.306 -37.639 0.26 – – –
Hunt & Reffert 2023 257.054 -37.547 0.262 -1.164 -2.309 -39.259

💡 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 – – – – – 22487* – –
Cavallo et al. 2024 3.77 4.69 – 129 -0.090 – – –
Hunt & Reffert 2023 3.35 4.23 3.21 590 – – – –

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

Visualization

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