HSC 1889

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0.37 UTI
0.3
CN
0.78
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 8.7 [arcmin]
  • CN 0.3 Poorly populated
  • Cdens 0.78 Dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1889 is a poorly populated, dense object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Relatively close Low extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 121.669 -17.361 0.911 -3.24 1.571 27.702
Hunt & Reffert 2024 121.715 -17.398 0.922 -3.247 1.602 26.375
Cavallo et al. 2024 121.677 -17.32 0.917 – – –
Hunt & Reffert 2023 121.715 -17.398 0.922 -3.247 1.602 26.375

💡 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 – – – – – 74* – –
Cavallo et al. 2024 1.07 0.01 – 389 0.320 – – –
Hunt & Reffert 2023 1.02 0.08 0.26 272 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3041 93.3 121.67 -17.36 0.91 -3.24 1.57 30.75 0.0

💡 Note: The % column shows the percentage of members that HSC 1889 shares with each listed object.

Visualization

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