HSC 179

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0.15 UTI
0.0
CN
0.02
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 5.1 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.02 Very loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 179 is a sparse, very loose object of high C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by high extinction. It is catalogued as an extremely massive, near-solar metallicity, old 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.

Very distant High extinction Extremely massive Near-solar metallicity Old

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 – 272.342 -15.262 0.117 -3.491 -6.585 105.532
Hunt & Reffert 2024 272.344 -15.25 0.116 -3.458 -6.606 77.63
Cavallo et al. 2024 272.326 -15.28 0.115 – – –
Hunt & Reffert 2023 272.344 -15.25 0.116 -3.458 -6.606 77.63

💡 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 – – – – – 28246* – –
Cavallo et al. 2024 6.14 3.65 – 2754 -0.080 – – –
Hunt & Reffert 2023 7.25 4.66 2.33 3327 – – – –

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

Visualization

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