HSC 1726

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0.46 UTI
0.28
CN
1.0
Cdens
1.0
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 0.6 [arcmin]
  • CN 0.28 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 1726 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a very small percentage of members with a later reported entry. See table with shared members information.

Very distant Moderate extinction Near-solar metallicity Intermediate age

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 – 101.879 -6.38 0.131 -0.365 0.529 –
Hunt & Reffert 2024 101.881 -6.381 0.091 -0.288 0.503 –
Cavallo et al. 2024 101.867 -6.286 0.091 – – –
Hunt & Reffert 2023 101.881 -6.381 0.091 -0.288 0.503 –

💡 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 – – – – – 215* – –
Cavallo et al. 2024 4.81 1.08 – 123 0.110 – – –
Hunt & Reffert 2023 8.21 1.24 1.07 83 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 4028 7.1 102.0 -6.3 0.11 -0.19 0.56 61.53 0.07

💡 Note: The % column shows the percentage of members that HSC 1726 shares with each listed object.

Visualization

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