HSC 687

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0.25 UTI
0.0
CN
0.61
Cdens
0.62
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 9.4 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.61 Moderately dense
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 687 is a sparse, moderately dense object of intermediate C3 quality. Its parallax locates it at a close 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.
Close Moderate extinction Near-solar metallicity Young

Cavallo et al. (2024)
Silver 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 – 314.587 46.836 1.066 -2.352 -6.175 -5.504
Cavallo et al. 2024 315.219 46.437 1.069 – – –
Hunt & Reffert 2023 314.582 46.812 1.069 -2.302 -6.288 -17.456

💡 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 0.93 1.56 – 93 0.240 – – –
Hunt & Reffert 2023 0.91 1.88 1.83 49 – – – –

Visualization

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