HSC 616

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0.09 UTI
0.0
CN
0.18
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 17.5 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.18 Very loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 616 is a sparse, very loose object of low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

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.

Close Moderate extinction Near-solar metallicity Young

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 308.744 39.195 0.994 1.568 -0.106 -6.08
Zhang et al. 2024 308.597 38.9 – – – –
Cavallo et al. 2024 308.9 39.359 0.99 – – –
Hunt & Reffert 2023 308.597 38.9 0.979 1.5 -0.096 -3.615

💡 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
Zhang et al. 2024 – – – – -0.131* – – –
Cavallo et al. 2024 1.03 2.10 – 40 -0.030 – – –
Hunt & Reffert 2023 0.95 1.68 1.84 132 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 4120 88.0 308.87 39.48 1.01 1.58 -0.08 -5.5 0.09

💡 Note: The % column shows the percentage of members that HSC 616 shares with each listed object.

Visualization

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