HSC 2679

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0.00 UTI
0.0
CN
0.87
Cdens
0.75
CC3
0.0
Clit
0.0
Cdup
Radius (P>50% members) 2.2 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.87 Dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.0 Very likely duplicate

Overview

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HSC 2679 is a sparse, dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by very high extinction. It is catalogued as a massive, near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry, and a moderate percentage with at least one entry reported in the same catalogue. See table with shared members information.

Relatively close Very high extinction Massive Near-solar metallicity Young

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 – 226.178 -58.488 0.291 -4.995 -3.469 -62.783
Hunt & Reffert 2024 226.159 -58.495 0.287 -4.981 -3.481 -64.3
Cavallo et al. 2024 226.174 -58.494 0.287 – – –
Hunt & Reffert 2023 226.159 -58.495 0.287 -4.981 -3.481 -64.3

💡 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 – – – – – 2143* – –
Cavallo et al. 2024 2.54 5.36 – 83 0.130 – – –
Hunt & Reffert 2023 3.25 5.66 1.52 68 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 265 100.0 226.18 -58.49 0.3 -4.94 -3.48 -62.07 0.49
HSC 2680 44.0 226.18 -58.5 0.34 -4.97 -3.55 -46.68 0.0
MCM 58 24.0 226.1 -58.54 0.35 -5.06 -3.4 -2.93 0.12

💡 Note: The % column shows the percentage of members that HSC 2679 shares with each listed object.

Visualization

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