HSC 693

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0.26 UTI
0.26
CN
0.65
Cdens
0.5
CC3
0.0
Clit
0.92
Cdup
Radius (P>50% members) 25.2 [arcmin]
  • CN 0.26 Poorly populated
  • Cdens 0.65 Moderately dense
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.92 Very likely unique

Overview

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HSC 693 is a poorly populated, moderately dense object of intermediate C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

Note: This is very likely a unique object, which shares a very small percentage of members with at least one previously reported entry. See table with shared members information.

Very close Low extinction Near-solar metallicity Young

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 314.612 47.439 2.598 4.715 0.541 -6.328
Cavallo et al. 2024 314.607 47.476 2.626 – – –
Hunt & Reffert 2023 314.683 47.538 2.627 4.755 0.55 -8.528

💡 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
Cavallo et al. 2024 0.40 0.51 – 20 0.090 – – –
Hunt & Reffert 2023 0.37 0.08 0.26 42 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1045 7.7 314.27 46.3 2.67 5.8 1.22 -11.91 0.09

💡 Note: The % column shows the percentage of members that HSC 693 shares with each listed object.

Visualization

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