HSC 1897

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0.32 UTI
0.57
CN
0.28
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 35.5 [arcmin]
  • CN 0.57 Moderately populated
  • Cdens 0.28 Loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1897 is a moderately populated, loose object of high C3 quality. Its parallax locates it at a 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.
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 – 115.129 -21.343 1.518 -5.988 4.222 36.126
Cavallo et al. 2024 114.693 -21.029 1.525 – – –
Hunt & Reffert 2023 115.148 -21.553 1.516 -5.989 4.184 36.515

💡 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 0.69 0.27 – 23 0.190 – – –
Hunt & Reffert 2023 0.63 0.12 0.59 89 – – – –

Visualization

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