HSC 427

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0.25 UTI
0.25
CN
0.48
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 48.1 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 0.48 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 427 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a very close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.
Very close Low extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 317.104 1.788 4.333 13.214 -7.951 5.82
Zhang et al. 2024 316.836 1.943 – – – –
Cavallo et al. 2024 317.458 1.673 4.397 – – –
Hunt & Reffert 2023 316.836 1.943 4.363 13.2 -7.876 2.237

💡 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 – – – – -0.059* – – –
Cavallo et al. 2024 0.23 0.49 – 240 0.250 – – –
Hunt & Reffert 2023 0.23 0.18 0.78 156 – – – –

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

Visualization

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