HSC 353

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0.20 UTI
0.0
CN
0.62
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 3.5 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.62 Moderately dense
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 353 is a sparse, moderately dense object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by very high extinction. It is catalogued as a metal-poor, 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 Very high extinction Metal-poor Young

Cavallo et al. (2024)
Bronze sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 286.097 4.608 0.366 -1.652 -2.632 31.926
Hunt & Reffert 2024 286.101 4.613 0.38 -1.628 -2.628 17.749
Cavallo et al. 2024 286.096 4.598 0.381 – – –
Hunt & Reffert 2023 286.101 4.613 0.38 -1.628 -2.628 17.749

💡 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 – – – – – 616* – –
Cavallo et al. 2024 2.68 5.84 – 47 -0.590 – – –
Hunt & Reffert 2023 2.34 6.36 2.54 55 – – – –

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

Visualization

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