HSC 1467

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0.27 UTI
0.0
CN
0.21
Cdens
0.62
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 14.7 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.21 Very loose
  • CC3 0.62 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 1467 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a low-mass, 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.
Close Moderate extinction Low mass 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 – 93.347 26.55 1.101 1.007 -1.734 -7.364
Zhang et al. 2024 93.241 26.565 – – – –
Hunt & Reffert 2024 93.241 26.565 1.109 1.037 -1.781 -12.877
Cavallo et al. 2024 93.338 26.523 1.119 – – –
Hunt & Reffert 2023 93.241 26.565 1.109 1.037 -1.781 -12.877

💡 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 – – – – -0.097* – – –
Hunt & Reffert 2024 – – – – – 49* – –
Cavallo et al. 2024 0.98 1.11 – 79 0.610 – – –
Hunt & Reffert 2023 0.87 0.95 0.39 166 – – – –

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

Visualization

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