HSC 934

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0.05 UTI
0.36
CN
0.29
Cdens
0.75
CC3
0.0
Clit
0.17
Cdup
Radius (P>50% members) 4.0 [arcmin]
  • CN 0.36 Poorly populated
  • Cdens 0.29 Loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.17 Likely duplicate

Overview

â„šī¸
HSC 934 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a moderate distance, near 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 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 – 359.894 62.444 0.233 -1.248 -0.692 -66.844
Hunt & Reffert 2024 359.897 62.44 0.233 -1.248 -0.693 -52.245
Cavallo et al. 2024 359.905 62.451 0.236 – – –
Hunt & Reffert 2023 359.897 62.44 0.233 -1.248 -0.693 -52.245

💡 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 – – – – – 315* – –
Cavallo et al. 2024 3.30 1.60 – 251 0.240 – – –
Hunt & Reffert 2023 3.68 1.57 1.80 207 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 595 83.3 359.88 62.44 0.23 -1.25 -0.69 -66.84 0.27

💡 Note: The % column shows the percentage of members that HSC 934 shares with each listed object.

Visualization

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