HSC 338

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0.05 UTI
0.0
CN
0.15
Cdens
0.12
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 6.1 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.15 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 338 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, metal-rich, young 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.

Relatively close High extinction Massive Metal-rich Young

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 – 283.633 2.875 0.406 -0.6 -2.662 -45.505
Hunt & Reffert 2024 283.636 2.902 0.429 -0.637 -2.685 49.026
Cavallo et al. 2024 283.74 2.884 0.449 – – –
Hunt & Reffert 2023 283.636 2.902 0.429 -0.637 -2.685 49.026

💡 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 – – – – – 4535* – –
Cavallo et al. 2024 2.87 4.86 – 38 0.720 – – –
Hunt & Reffert 2023 1.88 4.37 3.12 119 – – – –

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

Visualization

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