HSC 1967

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0.27 UTI
0.0
CN
0.58
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 2.2 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.58 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1967 is a sparse, moderately dense 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, young cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Distant Moderate extinction Near-solar metallicity Young

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 – 118.02 -27.669 0.227 -2.459 3.164 –
Hunt & Reffert 2024 118.008 -27.666 0.205 -2.444 3.151 –
Cavallo et al. 2024 118.014 -27.623 0.203 – – –
Hunt & Reffert 2023 118.008 -27.666 0.205 -2.444 3.151 –

💡 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 – – – – – 202* – –
Cavallo et al. 2024 3.39 1.60 – 15 -0.340 – – –
Hunt & Reffert 2023 4.45 1.67 0.60 83 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3564 100.0 118.02 -27.66 0.22 -2.46 3.15 96.13 0.16

💡 Note: The % column shows the percentage of members that HSC 1967 shares with each listed object.

Visualization

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