HSC 550

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0.11 UTI
0.0
CN
0.03
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 5.6 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.03 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 550 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by high extinction. It is catalogued as a 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 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 – 302.183 30.737 0.174 -2.793 -4.616 -24.91
Hunt & Reffert 2024 302.155 30.755 0.184 -2.772 -4.611 -24.936
Cavallo et al. 2024 302.188 30.723 0.191 – – –
Hunt & Reffert 2023 302.155 30.755 0.184 -2.772 -4.611 -24.936

💡 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 – – – – – 1279* – –
Cavallo et al. 2024 5.35 4.85 – 81 0.090 – – –
Hunt & Reffert 2023 4.64 4.91 2.44 429 – – – –

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

Visualization

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