HSC 2776

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0.16 UTI
0.32
CN
0.21
Cdens
0.5
CC3
0.0
Clit
0.78
Cdup
Radius (P>50% members) 6.8 [arcmin]
  • CN 0.32 Poorly populated
  • Cdens 0.21 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.78 Very likely unique

Overview

â„šī¸
HSC 2776 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a moderate 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 is very likely a unique object, which shares a 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=0.78) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Relatively close Moderate 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 – 246.064 -48.865 0.357 -1.361 -2.845 -34.702
Hunt & Reffert 2024 246.165 -48.824 0.355 -1.418 -2.87 –
Cavallo et al. 2024 246.124 -48.817 0.349 – – –
Hunt & Reffert 2023 246.165 -48.824 0.355 -1.418 -2.87 –

💡 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 – – – – – 559* – –
Cavallo et al. 2024 1.98 2.88 – 9 -0.450 – – –
Hunt & Reffert 2023 2.50 2.68 2.74 48 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 4126 53.1 246.14 -48.79 0.35 -1.27 -2.78 -32.71 0.17
CWNU 2395 21.9 245.65 -49.17 0.38 -1.42 -2.93 -27.98 0.35

💡 Note: The % column shows the percentage of members that HSC 2776 shares with each listed object.

Visualization

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