HSC 884

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0.39 UTI
0.45
CN
0.77
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 14.9 [arcmin]
  • CN 0.45 Poorly populated
  • Cdens 0.77 Dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 884 is a poorly populated, dense object of high 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, very young cluster (see Parameters). It was recently reported in the literature.
Close Moderate extinction Near-solar metallicity Very young

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 348.488 61.799 1.27 -1.227 -2.945 -15.377
Hunt & Reffert 2024 348.28 61.712 1.271 -1.194 -2.829 -14.574
Cavallo et al. 2024 348.496 61.972 1.276 – – –
Hunt & Reffert 2023 348.28 61.712 1.271 -1.194 -2.829 -14.574

💡 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 – – – – – 51* – –
Cavallo et al. 2024 0.82 1.36 – 6 -0.200 – – –
Hunt & Reffert 2023 0.75 1.23 2.19 7 – – – –

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

Visualization

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