HSC 2717

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0.05 UTI
0.5
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.12
Cdup
Radius (P>50% members) 2.2 [arcmin]
  • CN 0.5 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.12 Likely duplicate

Overview

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HSC 2717 is a moderately populated, very dense object of 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, metal-rich, old cluster (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Distant Very high extinction Massive Metal-rich Old

Cavallo et al. (2024)
Wood sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 233.207 -54.924 0.256 -4.995 -4.767 -58.467
Hunt & Reffert 2024 233.198 -54.931 0.28 -4.962 -4.707 –
Cavallo et al. 2024 233.232 -54.918 0.276 – – –
Hunt & Reffert 2023 233.198 -54.931 0.28 -4.962 -4.707 –

💡 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 – – – – – 1406* – –
Cavallo et al. 2024 4.37 5.17 – 5 0.910 – – –
Hunt & Reffert 2023 2.85 5.07 2.78 2360 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3862 100.0 233.21 -54.92 0.25 -5.01 -4.78 -43.31 0.09
LS 229 88.2 233.16 -54.95 0.29 -5.26 -4.84 -59.05 0.5

💡 Note: The % column shows the percentage of members that HSC 2717 shares with each listed object.

Visualization

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