HSC 2921

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0.09 UTI
0.0
CN
0.22
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 5.3 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.22 Very loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2921 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high 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 small 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.

Relatively close High extinction Near-solar metallicity Young

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 – 263.435 -35.012 0.385 -0.631 -2.082 118.215
Hunt & Reffert 2024 263.43 -35.02 0.392 -0.657 -2.102 -49.409
Cavallo et al. 2024 263.448 -35.051 0.392 – – –
Hunt & Reffert 2023 263.43 -35.02 0.392 -0.657 -2.102 -49.409

💡 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 – – – – – 824* – –
Cavallo et al. 2024 1.74 3.71 – 58 -0.090 – – –
Hunt & Reffert 2023 2.29 3.64 2.48 33 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3529 20.0 263.43 -35.02 0.35 -0.81 -2.32 -33.33 0.51

💡 Note: The % column shows the percentage of members that HSC 2921 shares with each listed object.

Visualization

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