HSC 914

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0.46 UTI
0.31
CN
1.0
Cdens
1.0
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 1.2 [arcmin]
  • CN 0.31 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 914 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a massive, metal-rich, 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.

Distant High extinction Massive Metal-rich 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 – 353.727 63.365 0.223 -1.941 -0.527 -84.936
Hunt & Reffert 2024 353.726 63.372 0.225 -1.941 -0.541 -84.938
Cavallo et al. 2024 353.75 63.364 0.225 – – –
Hunt & Reffert 2023 353.726 63.372 0.225 -1.941 -0.541 -84.938

💡 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 – – – – – 1019* – –
Cavallo et al. 2024 3.60 3.56 – 398 0.590 – – –
Hunt & Reffert 2023 3.81 4.29 2.34 258 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3362 100.0 353.73 63.37 0.22 -1.94 -0.52 -84.94 0.15

💡 Note: The % column shows the percentage of members that HSC 914 shares with each listed object.

Visualization

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