HSC 638

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0.27 UTI
0.32
CN
0.15
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 21.5 [arcmin]
  • CN 0.32 Poorly populated
  • Cdens 0.15 Very loose
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 638 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by high 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.
Relatively close High extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 310.422 41.707 0.968 2.528 -2.582 -11.22
Zhang et al. 2024 310.356 41.665 – – – –
Hunt & Reffert 2024 310.357 41.665 0.979 2.499 -2.567 -19.113
Cavallo et al. 2024 310.346 41.792 0.971 – – –
Hunt & Reffert 2023 310.357 41.665 0.979 2.499 -2.567 -19.113

💡 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 – – – – -0.035* – – –
Hunt & Reffert 2024 – – – – – 54* – –
Cavallo et al. 2024 1.05 3.25 – 105 -0.360 – – –
Hunt & Reffert 2023 1.00 3.11 1.91 136 – – – –

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

Visualization

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