HSC 674

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0.06 UTI
0.0
CN
0.11
Cdens
0.5
CC3
0.0
Clit
0.48
Cdup
Radius (P>50% members) 78.2 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.11 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.48 Possibly duplicate

Overview

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HSC 674 is a sparse, very loose 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.

âš ī¸ Warning: This is possibly a duplicate object, which shares a significant 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 – 317.04 47.634 3.41 7.019 0.629 -6.898
Cavallo et al. 2024 317.344 47.781 3.39 – – –
Hunt & Reffert 2023 314.156 45.68 3.391 7.021 0.67 -9.824

💡 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 0.30 0.59 – 11 -0.410 – – –
Hunt & Reffert 2023 0.30 0.30 0.55 33 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1021 52.0 318.6 48.93 3.32 7.18 0.81 -8.24 0.18

💡 Note: The % column shows the percentage of members that HSC 674 shares with each listed object.

Visualization

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