HSC 2724

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0.32 UTI
0.27
CN
1.0
Cdens
0.38
CC3
0.0
Clit
0.96
Cdup
Radius (P>50% members) 2.3 [arcmin]
  • CN 0.27 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.96 Unique

Overview

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HSC 2724 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a moderate distance, above 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 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.

Relatively close High extinction Near-solar metallicity 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 – 235.394 -53.979 0.464 -0.807 -0.924 -28.152
Hunt & Reffert 2024 235.402 -53.976 0.477 -0.768 -0.949 –
Cavallo et al. 2024 235.402 -53.988 0.477 – – –
Hunt & Reffert 2023 235.402 -53.976 0.477 -0.768 -0.949 –

💡 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 – – – – – 155* – –
Cavallo et al. 2024 1.78 3.61 – 43 0.150 – – –
Hunt & Reffert 2023 2.22 3.53 0.62 32 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
VVV 055 3.7 235.89 -54.0 0.44 -0.68 -0.82 -33.39 0.22

💡 Note: The % column shows the percentage of members that HSC 2724 shares with each listed object.

Visualization

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