HSC 2768

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0.45 UTI
0.25
CN
1.0
Cdens
1.0
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 0.7 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2768 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by very high extinction. It is catalogued as a massive, intermediate-age 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.

Distant Very high extinction Massive Intermediate age

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 243.921 -48.64 0.228 -2.875 -3.238 -69.26
Hunt & Reffert 2024 243.916 -48.645 0.219 -2.851 -3.24 -69.257
Hunt & Reffert 2023 243.916 -48.645 0.219 -2.851 -3.24 -69.257

💡 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 – – – – – 1150* – –
Hunt & Reffert 2023 4.29 5.50 1.88 163 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3777 92.0 243.92 -48.64 0.22 -2.88 -3.24 -69.26 0.05

💡 Note: The % column shows the percentage of members that HSC 2768 shares with each listed object.

Visualization

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