HSC 1029

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0.37 UTI
0.25
CN
0.34
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 14.3 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 0.34 Loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 1029 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a 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.
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 – 20.974 48.994 1.08 -5.868 -2.568 -31.123
Zhang et al. 2024 20.856 48.999 – – – –
Hunt & Reffert 2024 20.856 48.999 1.089 -5.801 -2.549 -31.974
Cavallo et al. 2024 21.047 48.955 1.081 – – –
Hunt & Reffert 2023 20.856 48.999 1.089 -5.801 -2.549 -31.974

💡 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
Zhang et al. 2024 – – – – 0.010* – – –
Hunt & Reffert 2024 – – – – – 52* – –
Cavallo et al. 2024 0.79 0.55 – 355 -0.030 – – –
Hunt & Reffert 2023 0.86 0.19 0.48 711 – – – –

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

Visualization

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