HSC 951

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0.20 UTI
0.0
CN
0.39
Cdens
0.62
CC3
0.0
Clit
0.96
Cdup
Radius (P>50% members) 5.4 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.39 Loose
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.96 Unique

Overview

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HSC 951 is a sparse, loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a metal-rich, very young cluster (see Parameters). It was recently reported in the literature.

Note: This is a unique object, which shares a very small percentage of members with at least one previously reported entry. See table with shared members information.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=0.96) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Relatively close High extinction Metal-rich Very young

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 4.545 65.827 0.481 -2.847 -0.108 8.8
Hunt & Reffert 2024 4.541 65.826 0.492 -2.854 -0.111 -32.06
Cavallo et al. 2024 4.649 65.85 0.49 – – –
Hunt & Reffert 2023 4.541 65.826 0.492 -2.854 -0.111 -32.06

💡 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 – – – – – 224* – –
Cavallo et al. 2024 2.17 3.94 – 5 0.830 – – –
Hunt & Reffert 2023 1.89 4.51 1.94 5 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Teutsch 168 4.0 4.81 65.84 0.37 -3.15 0.32 – 0.12

💡 Note: The % column shows the percentage of members that HSC 951 shares with each listed object.

Visualization

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