HSC 1638

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0.02 UTI
0.66
CN
0.91
Cdens
0.75
CC3
0.0
Clit
0.05
Cdup
Radius (P>50% members) 3.5 [arcmin]
  • CN 0.66 Moderately populated
  • Cdens 0.91 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.05 Very likely duplicate

Overview

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HSC 1638 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Distant Moderate 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 – 101.887 5.63 0.24 -0.639 -0.284 71.314
Hunt & Reffert 2024 101.889 5.631 0.243 -0.634 -0.296 58.24
Cavallo et al. 2024 101.893 5.627 0.237 – – –
Hunt & Reffert 2023 101.889 5.631 0.243 -0.634 -0.296 58.24

💡 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 – – – – – 589* – –
Cavallo et al. 2024 3.45 1.61 – 65 0.170 – – –
Hunt & Reffert 2023 3.40 1.37 2.37 213 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 1390 95.1 101.89 5.63 0.24 -0.63 -0.29 71.31 0.45
CWWDL 10880 81.7 101.9 5.64 0.24 -0.63 -0.28 93.37 0.06

💡 Note: The % column shows the percentage of members that HSC 1638 shares with each listed object.

Visualization

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