HSC 2729

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0.33 UTI
0.25
CN
0.65
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 6.2 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 0.65 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2729 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Relatively close Low 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 – 243.762 -59.005 0.652 -1.822 -0.823 -28.236
Hunt & Reffert 2024 243.762 -59.002 0.646 -1.82 -0.828 -37.398
Cavallo et al. 2024 243.741 -59.003 0.645 – – –
Hunt & Reffert 2023 243.762 -59.002 0.646 -1.82 -0.828 -37.398

💡 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 – – – – – 87* – –
Cavallo et al. 2024 1.58 0.80 – 117 0.050 – – –
Hunt & Reffert 2023 1.48 0.63 0.26 139 – – – –

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

Visualization

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